ARIHIP

Individual notes

1)     HIP    154 = FK 1630

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
R.M. Catchpole et al. (1982, Royal Obs. Bull. No. 188, 5)
claim from two measurements a variable radial velocity.
Many more observations by W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147) favour a constant radial velocity.


2)     HIP    301 = FK  905

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609).
Barbier-Brossat (1989) gives v_rad = +8 km/s (Field 17: -5 km/s).


3)     HIP    377 = FK 1001

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1961, Monthly Not. Roy. Astron. Soc.  123, 233).


4)     HIP    560 = FK 1003

   Radial velocity is variable according to BSC.


5)     HIP    950 = FK    6

   Radial velocity is variable according to J. Andersen and B. Nordstroem (1983,
Astron. Astrophys. 122, 23).


6)     HIP   1473 = FK 1005

   Radial velocity is variable, but this is probably due to pulsation
(E. Antonello et al., 1978, Astron. Astrophys. 66, 37).


7)     HIP   1562 = FK    9

   2 companions in CCDM+WDS:
B(1911:  63",  17 deg, 12.9 mag; af), C(1960: 109", 194 deg,  8.6 mag; nc).
TYCHO gives for C(1991: 108", 192 deg, 10.64 mag) and indicates also nc.


8)     HIP   1599 = FK   10

   The faint companion (rho ~31", 10.34 mag) listed in the TYCHO
Catalogue (ESA, 1997) is spurious and was caused by side-lobe interferences
from the bright FK star (V. Makarov, 1999, private communication).


9)     HIP   2006 = FK 1010

   Probably not a visual binary according to S.W. Burnham (1906, General
Catalogueof Double Stars). O. Struve (1878, Pulkova Obs. 9 (Object O_Sigma_8))
gave rho ~1" and m_B ~9.


10)    HIP   2224 = FK 1012

   Radial velocity is variable (e.g. R.K. Young, 1939,
Publ. David Dunlap Obs. Toronto, Vol. 1, No. 3, p. 71;
W.I. Beavers and J.J. Eitter, 1986, Astrophys. J. Suppl. Ser. 62, 147).


11)    HIP   2381 = FK   14

   Announced as a spectroscopic binary by W.S. Adams (1912, Astrophys. J.
35, 163  and Publ. Astron. Soc. Pacific  24, 129). Later observations
(e.g. J. Andersen and B. Nordstroem (1983, Astron. Astrophys. 122, 23))
do not confirm such radial-velocity variations. Doubtful case, mainly
because of the large rotational velocity v_rot sin(i) ~200 km/s.


12)    HIP   2599 = FK   16

   In spite of some reports on radial-velocity variations (e.g. BSC), the star
is probably not a spectroscopic binary (M.M. Jarad et al., 1989, Monthly Not.
Roy. Astron. Soc.  238, 1085).


13)    HIP   2661 = FK 1013

   Radial velocity is variable according to W.I. Beavers and J.J. Eitter (1986,
Astrophys. J. Suppl. Ser. 62, 147).


14)    HIP   2920 = FK   17

   Radial velocity may be variable according to BSC.
H. Sadsaoud et al. (1994, Astron. Astrophys.  287, 509) propose a close binary
with a period of 11.53 days and an amplitude of a few km/s.
The duplicity is doubtful.


15)    HIP   3245 = FK 1015

   Radial velocity may be variable according to BSC.


16)    HIP   3419 = FK   22

   Radial velocity may be variable according to K.A. Murdoch et al. (1993,
Astrophys. J. 413, 349).


17)    HIP   3521 = FK 1017

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609) and to W. Buscombe
(1963, Monthly Not. Roy. Astron. Soc.  126, 29).


18)    HIP   3781 = FK   31

   Radial velocity is variable according to BSC.
Suspicion of variable radial velocity not supported by
D.S. Evans et al. (1964, Royal Obs. Bull. No. 85).


19)    HIP   3786 = FK   28

   1 companion in CCDM+WDS:
B(1960: 113",  14 deg, 13.2 mag; nc).
Radial velocity may be variable according to BSC.


20)    HIP   3909 = FK   30

   Radial velocity is variable according to BSC.


21)    HIP   4293 = FK   34

   Sinzi (1972) indicates an optical companion.
We were unable to identify such a star.


22)    HIP   4577 = FK   35

   Radial velocity is variable according to BSC.


23)    HIP   4592 = FK 1024

   Radial velocity is variable according to J. Andersen and B. Nordstroem (1983,
Astron. Astrophys. Suppl. Ser. 52, 479).


24)    HIP   4852 = FK 1026

   Radial velocity is variable
according to W. Buscombe (1963, Monthly Not. Roy. Astron. Soc.  126, 29)
and to P.A. Wayman (1961, Royal Obs. Bull. No. 36).


25)    HIP   5364 = FK   40

   1 companion in CCDM+WDS:
B(1908: 234", 305 deg, 10.3 mag; af).
TYCHO gives for B(1991: 254", 305 deg, 10.78 mag).


26)    HIP   5586 = FK   43

   Radial velocity may be variable (W.W. Campbell, 1928, Publ. Lick Obs.  16,
15; G.H. Herbig and J.F. Spalding, 1955, Astrophys. J. 121, 118).


73",  94 deg,27)    HIP   5626 = FK   41

   Barbier-Brossat (1989) gives v_rad = +10 km/s (Field 17: +18 km/s).


28)    HIP   5661 = FK   44

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609)
and to W. Buscombe (1963, Monthly Not. Roy. Astron. Soc.  126, 29).
Delta Scuti star AI Scl. The pulsation explains the radial-velocity variations.


29)    HIP   6061 = FK 1034

   Radial velocity is variable according to BSC.


30)    HIP   6193 = FK   45

   Radial velocity is variable according to BSC.


31)    HIP   6411 = FK 1035

   Radial velocity is probably variable according to W.I. Beavers
(1985, IAU Colloquium No. 88, p. 289). Later, W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147) consider the radial velocity
as essentially constant. Sinzi (1972) claims that the star is an
eclipsing binary. This information is probably spurious.


32)    HIP   6537 = FK   47

   1 companion in CCDM+WDS:
B(1925:  65",  57 deg, 14.8 mag; af).


33)    HIP   6686 = FK   48

   1 companion in CCDM+WDS:
B(1925: 132",  66 deg, 11.5 mag; af).
Eclipsing binary with a possible period of 759 days.
Radial velocity is variable according to BSC and WDS.


34)    HIP   6732 = FK 1039

   Radial velocity is variable according to BSC.


35)    HIP   7083 = FK 1044

   Radial velocity is possibly slightly variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


36)    HIP   7513 = FK 1045

   2 companions in CCDM+WDS:
B(1910: 114", 128 deg, 12.6 mag; af), C(1926: 291", 283 deg,  9.  mag; af).
The spectroscopic-binary orbit provided by H.A. Abt and S.G. Levy (1976,
Astrophys. J. Suppl. Ser. 30, 273) is spurious, since this radial-velocity variation
was not confirmed by A. Duquennoy and M. Mayor (1991, Astron. Astrophys.
248, 485). The star has probably three planets (R.P. Butler et al., 1997,
Astrophys. J. 474, L115; G.W. Marcy et al., 1999, Bull. American
Astron. Soc.  194, No. 14.02).


37)    HIP   7941 = FK   58

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233) and to P.A. Wayman (1961, Royal Obs. Bull. No. 36).


38)    HIP   7943 = FK 1047

   Radial velocity is variable according to BSC.


39)    HIP   8102 = FK   59

   1 companion in CCDM+WDS:
B(1940:  90", 215 deg, 13.1 mag; af).
The radial velocity is constant
(B. Campbell et al., 1988, Astrophys. J. 331, 902;
G.A.H. Walker et al., 1995, Icarus  116, 359;
A.P. Hatzes et al., 1996, J. Geophys. Research  101, 9285).


40)    HIP   8387 = FK 1050

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


41)    HIP   8837 = FK   67

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable (H. Spencer Jones, 1928, Ann. Cape Obs.
10, part 8, 95).


42)    HIP   8886 = FK   63

   Radial velocity is variable according to BSC.


43)    HIP   9505 = FK 1054

   Radial velocity is variable according to BSC.


44)    HIP   9598 = FK   70

   Double-lined spectroscopic binary according to BSC.


45)    HIP   9884 = FK   74

   Probably not a spectroscopic binary in spite of earlier claims (W. Schaub,
1932, Z. f. Astrophys. 4, 35).


46)    HIP  10155 = FK 1056

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC.


47)    HIP  10320 = FK   78

   Radial velocity is variable according to
W. Buscombe and P.M. Morris (1961, Monthly Not. Roy. Astron. Soc.  123, 233) or
may be variable according to D.S. Evans et al. (1964, Royal Obs. Bull. No. 85).


48)    HIP  10328 = FK 1057

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


49)    HIP  10440 = FK 1060

   Suspicion of variable radial velocity (W. Buscombe and P.M. Morris, 1958,
Monthly Not. Roy. Astron. Soc.  118, 609).


50)    HIP  10602 = FK   82

   1 companion in CCDM+WDS:
B(1985:  88", 223 deg,  9.0 mag; af).
TYCHO gives for B(1991:  89", 223 deg, 9.73 mag).


51)    HIP  10642 = FK   80

   Radial velocity may be variable according to BSC.


52)    HIP  10670 = FK   79

   Radial velocity is variable according to BSC.


53)    HIP  10732 = FK   81

   Radial velocity is variable according to GCRV and BSC.


54)    HIP  10819 = FK 1063

   Radial velocity is assumed to be variable  by
W.S. Adams (1912, Publ. Astron. Soc. Pacific  24, 129),
W.W. Campbell and J.H. Moore (1928, Publ. Lick Obs.  16, 27),
W.E.Harper  (1937, Publ. Dominion Astrophys. Obs. 7, 1), and BSC,
but not by GCRV. Duplicity doubtful.


55)    HIP  10993 = FK 1656

   Double-lined spectroscopic binary according to J. Andersen and B. Nordstroem
(1977, Astron. Astrophys. Suppl. Ser. 29, 309).
More information is given by B. Nordstroem and J. Andersen
(1985, Astron. Astrophys. Suppl. Ser. 61, 53).


56)    HIP  11001 = FK 1065

   Radial velocity may be variable according to BSC.


57)    HIP  11258 = FK   84

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


58)    HIP  11345 = FK 1066

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


59)    HIP  11407 = FK   86

   Radial velocity may be variable according to BSC.


60)    HIP  11486 = FK 1068

   Radial velocity is variable according to BSC.


61)    HIP  11698 = FK 1069

   Radial velocity is variable (R. Woolley, G.A. Harding, 1965, Roy. Obs. Bull.
No. 93; W.I. Beavers and J.J. Eitter, 1986, Astrophys. J. Suppl. Ser. 62, 147).


62)    HIP  11783 = FK 1071

   Radial velocity is variable according to J.Andersen and B. Nordstroem
(1983, Astron. Astrophys. 122, 23).


63)    HIP  12107 = FK 1074

   2 companions in CCDM+WDS:
B(1912: 117", 123 deg, 13.3 mag; pc), C(1912: 146", 189 deg,  9.3 mag; pc).


64)    HIP  12387 = FK   91

   Radial velocity is variable (pulsating Beta Cephei star). Weak indications of
binarity are discussed by M.C. Lane (1977, Publ. Astron. Soc. Pacific 89, 905).


65)    HIP  12768 = FK 1077

   Radial velocity may be variable according to
G. Burki and M. Mayor (1983, Astron. Astrophys. 124, 256).


66)    HIP  12770 = FK   97

   Radial velocity may be variable (J.A. Morse, 1991, Astron. J.  101, 1495).


67)    HIP  13327 = FK 1079

   Radial velocity is variable according to BSC.


68)    HIP  13717 = FK 1080

   Radial velocity may be variable
according to W.E. Harper (1937, Publ. Dominion Astrophys. Obs. 7, 1).
HIP: goodness-of-fit parameter F2 = 3.51.


69)    HIP  14117 = FK 1084

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


70)    HIP  14135 = FK  107

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


71)    HIP  14146 = FK 1085

   Radial velocity may be variable according to BSC.


72)    HIP  14187 = FK 1086

   Radial velocity is variable according to W. Buscombe (1963, Monthly Not.
Roy. Astron. Soc.  126, 29).


73)    HIP  14354 = FK  109

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


74)    HIP  14632 = FK  112

   1 companion in CCDM+WDS:
B(1912: 146", 132 deg, 12.4 mag; oo).
The motion of A is non-linear according to W.D. Heintz
(1988, Astron. J.  96, 1072), who suggests an orbital period of 6.5 years.
However, the rather low values of the test parameter F do not reveal a
non-linear motion of A.
In spite of earlier suspicions (BSC) is the radial velocity constant
(H.A. Abt and S.G. Levy, 1976, Astrophys. J. Suppl. Ser. 30, 273;
B. Campbell et al., 1988, Astrophys. J. 331, 902;
G.A.H. Walker et al., 1995, Icarus  116, 359).


75)    HIP  14677 = FK 1088

   Radial velocity is variable according to BSC.


76)    HIP  14838 = FK  114

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


77)    HIP  14930 = FK  118

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


78)    HIP  15110 = FK 1089

   Radial velocity is variable according to BSC.


79)    HIP  15201 = FK 1095

   Radial velocity is variable according to BSC.


80)    HIP  15265 = FK 1092

   Radial velocity is variable according to B. Nordstroem and J. Andersen
(1985, Astron. Astrophys. Suppl. Ser. 61, 53).


81)    HIP  15457 = FK 1093

   2 companions in CCDM+WDS:
B(1909: 269", 157 deg,  9.6 mag; af), C(BC: 1909: 215", 272 deg, 11.9 mag; oo).
A. Duquennoy and M. Mayor (1991, Astron. Astrophys. 248, 485)
suspected a radial-velocity variation.
According to G.A.H. Walker et al. (1995, Icarus  116, 359), this variation may
be connected to the chromospheric activity of the star.


82)    HIP  15863 = FK  120

   1 companion in CCDM+WDS:
B(1924: 167", 196 deg, 11.9 mag; nc, pc).
Radial velocity is variable according to BSC.


83)    HIP  15890 = FK 1096

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


84)    HIP  16341 = FK 1097

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.


85)    HIP  16509 = FK  128

   Radial velocity is variable according to W. Buscombe and  P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609).

86)    HIP  16518 = FK 1098

   Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity. Radial velocity is variable according to BSC.

87)    HIP  17304 = FK  133

   Radial velocity is variable according to BSC.


88)    HIP  17457 = FK  137

   Radial velocity is variable according to W. Buscombe (1963, Monthly Not. Roy.
Astron. Soc.  126, 29).


89)    HIP  17678 = FK  146

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


90)    HIP  18170 = FK 1106

   Radial velocity may be variable according to BSC.


91)    HIP  18217 = FK 1105

   1 companion in TYCHO:
B(1991:  67", 88 deg,  9.95 mag; oo).
Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity.


92)    HIP  18614 = FK  148

   Probably not a spectroscopic binary. Large variation in the radial velocity
may be due to a stellar wind (B. Bohannan and C.D. Garmany, 1978, Astrophys.
J. 223, 908).


93)    HIP  18788 = FK 1111

   Radial velocity is variable according to BSC.


94)    HIP  18907 = FK  151

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


95)    HIP  19038 = FK 1112

   2 companions in CCDM+WDS:
B(1926: 138",  10 deg,  9.5 mag; hv), C(1923: 235", 213 deg; ~oo).


96)    HIP  19095 = FK  153

   Radial velocity is variable according to BSC.


97)    HIP  19167 = FK 1113

   Radial velocity may be variable according to BSC.


98)    HIP  19388 = FK 1115

   Radial velocity is variable according to BSC.


99)    HIP  19513 = FK 1116

   Delta Scuti star IM Tau. The pulsation explains
the observed radial-velocity variations
(e.g. M.A. Smith, 1982, Astrophys. J. 254, 242).


100)   HIP  19587 = FK  154

   Delta Scuti star. The pulsation explains
the observed radial-velocity variations.


101)   HIP  19860 = FK 1118

   Radial velocity may be variable according to BSC.
HIP: percentage of rejected data F1 = 4%.


102)   HIP  19893 = FK  157

   Radial velocity may be variable according to BSC. Prototype of the
Gamma-Doradus-class of variable stars. Probably a pulsating star (L.A. Balona et al.,
1994, Monthly Not. Roy. Astron. Soc.  267, 103 and  270, 905).


103)   HIP  20049 = FK  166

   Radial velocity is variable (F.J. Neubauer, 1930, Lick Obs. Bull.  15, 46).
Composite spectrum (K2-3III+A) according to G.T. Davidson et al. (1987,
Astron. J. 94, 771).


104)   HIP  20252 = FK  158

   1 companion in CCDM+WDS:
B(1914: 110", 313 deg, 13.0 mag; oo).


105)   HIP  20264 = FK  161

   Radial velocity is variable according to BSC.


106)   HIP  20384 = FK  163

   1 companion in TYCHO:
B(1991:  86", 295 deg, 10.89 mag; oo).


107)   HIP  20507 = FK 1120

   Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity. Radial velocity may be variable according to BSC.


108)   HIP  20884 = FK 1123

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


109)   HIP  20889 = FK  164

   1 companion in CCDM+WDS:
B(1910: 182", 268 deg, 10.6 mag; oo).


110)   HIP  20974 = FK 1122

   Radial velocity is probably variable (D. Crampton and W. Morrison, 1979,
Publ. Astron. Soc. Pacific  91, 695).


111)   HIP  21242 = FK 1124

   3 companions in CCDM+WDS:
B(1914: 116", 198 deg,  6.8 mag; nc), C(1909: 104", 225 deg, 13.4 mag; oo),
D(1909:  76", 354 deg, 12.1 mag; oo).
B is HIP 21238 (1991: 120", 198 deg,  6.80 mag; hv).
Radial velocity is variable according to BSC.


112)   HIP  21743 = FK 1127

   Radial velocity is variable (F.J. Neubauer, 1930, Lick Obs. Bull.  15, 46;
H.A. Abt, 1970, Astrophys. J. Suppl. Ser. 19, 19).


113)   HIP  21861 = FK 1130

   Radial velocity may be variable according to BSC.


114)   HIP  21949 = FK  177

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.


115)   HIP  22361 = FK  173

   1 companion in CCDM+WDS:
B(1914:  97",  60 deg, 12.0 mag; oo).
TYCHO gives for another companion : (1991:  62", 206 deg, 11.06 mag; oo).
Radial velocity is variable according to BSC.


116)   HIP  22449 = FK 1134

   1 companion in CCDM+WDS:
B(1924:  90", 143 deg,  8.8 mag; af).
TYCHO gives B(1991: 76", 163 deg, 10.57 mag).
A is a spectroscopic binary according to WDS (SB) and BSC (SB2).
However, H.A. Abt and S.G. Levy (1976, Astrophys. J. Suppl. Ser. 30, 273)
and A. Duquennoy and M. Mayor (1991, Astron. Astrophys. 248, 485)
do not find variations in the radial velocity.


117)   HIP  22453 = FK 1133

   Radial velocity may be variable according to BSC.


118)   HIP  22565 = FK 1135

   1 companion in CCDM+WDS:
B(1963: 177", 302 deg, 10.4 mag; nc).
Radial velocity is variable according to BSC.
Delta Scuti star V480 Tau. The pulsation explains the radial-velocity variations.

119)   HIP  23522 = FK  182

   2 companions in CCDM+WDS:
B(1976:  83", 209 deg,  7.4 mag; pc, hv), C(BC: 1919:  15", 168 deg, 12.4 mag).
TYCHO gives for B(1991: 83", 209 deg,  7.39 mag).


120)   HIP  23607 = FK 1140

   Radial velocity is variable according to BSC.


121)   HIP  23767 = FK  185

   Radial velocity may be variable according to BSC.
K. Kodaira (1971, Publ. Astron. Soc. Japan  23, 159) suspected an orbital period
of about 24 days. H.A. Abt and S.G. Levy (1978, Astrophys. J. Suppl Ser. 36, 241)
did not confirm the binarity of this object.


122)   HIP  23875 = FK  188

   1 companion in CCDM+WDS:
B(1908: 117", 142 deg, 10.9 mag; af).
Radial velocity is variable according to Sinzi (1972).


123)   HIP  23972 = FK  190

   Beta Cephei star.
Radial velocity is variable according to H.A. Abt and S.G. Levy
(1978, Astrophys. J. Suppl. Ser. 36, 241). C.T. Bolton (1982, IAU Symp. 98,
181) explains the radial-velocity variations by pulsation of Lambda Eri.


124)   HIP  24372 = FK  196

   Radial velocity is variable according to BSC.


125)   HIP  24659 = FK  197

   Radial velocity may be variable according to BSC.


126)   HIP  24813 = FK 1145

   7 companions in CCDM+WDS:
B(1900:  29", 274 deg, 13.4 mag; af), C(1934:  42", 268 deg, 12.1 mag; af),
D(1921: 147",   2 deg,  8.6 mag; af),
E(DE: 1914: 146", 112 deg,  9.9 mag; unclear),
F(1921:  93", 211 deg, 11.1 mag; af),
G(EG: 1893:  33", 218 deg, 10.9 mag; af), H(EH: 1914: 147", 119 deg, 10.7 mag; af).
INCA gives
B(106", 310 deg, 13.4 mag), C( 87", 299 deg, 12.1 mag),
D(202", 350 deg,  8.6 mag), E(DE: 145", 113 deg,  9.9 mag),
F( 93", 253 deg, 11.1 mag), G(EG:  33", 216 deg, 10.9 mag),
H(EH: 147", 119 deg, 10.7 mag).
At present, all the companions have a separation rho with respect to A of more
than 60".


127)   HIP  25336 = FK  201

   1 companion in CCDM+WDS:
B(1909: 180", 144 deg, 12.2 mag; nc, hv).
Radial velocity may be variable according to BSC.


128)   HIP  25769 = FK  203

   1 companion in TYCHO:
B(1991:  66", 130 deg,  9.14 mag; pc).
Radial velocity may be variable according to BSC.


129)   HIP  25911 = FK 1637

   The radial velocity is variable
according to GCRV, BSC, and Sinzi (1972).


130)   HIP  25973 = FK 1150

   Radial velocity may be variable according to BSC.


131)   HIP  26311 = FK  210

   1 companion in CCDM+WDS:
B(1908: 180",  57 deg, 10.5 mag; pc).
Radial velocity is variable according to BSC.
While H. Levato et al. (1988, Astrophys. J. Suppl Ser. 68, 319) tend to confirm
the radial-velocity variations, the measurements by M.M. Jarad et al. (1989,
Monthly Not. Roy. Astron. Soc.  238, 1085) favour a constant radial velocity.


132)   HIP  26638 = FK  205

   Radial velocity may be variable according to BSC.


133)   HIP  27288 = FK  219

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC.


134)   HIP  27366 = FK  220

   Radial velocity may be variable according to BSC.
Beta Cephei star.


135)   HIP  27621 = FK 1159

   1 companion in TYCHO:
B(1991:  90", 294 deg, 10.26 mag; oo).


136)   HIP  27628 = FK  223

   Radial velocity is variable according to BSC.


137)   HIP  27949 = FK 1157

   Radial velocity may be variable according to BSC.


138)   HIP  28532 = FK 1638

   Radial velocity is variable according to BSC.


139)   HIP  28814 = FK  230

   Radial velocity may be variable according to BSC.


140)   HIP  28899 = FK 1164

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


141)   HIP  29134 = FK 1166

   Radial velocity may be variable according to BSC.


142)   HIP  29490 = FK  233

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


143)   HIP  29997 = FK  234

   Radial velocity is variable according to BSC.


144)   HIP  30324 = FK  243

   1 companion in CCDM+WDS:
B(1908: 186", 340 deg,  9.8 mag; nc, pc).
Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.
Beta Cephei star.

145)   HIP  30343 = FK  241

   3 companions in CCDM+WDS:
B(1899: 122", 141 deg,  9.8 mag; nc, hv), C(BC: 1939:   1", 260 deg, 10.7 mag),
D(1880:  73",  77 deg, 11.5 mag; oo).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


146)   HIP  30438 = FK  245

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is possibly slightly variable according to W. Buscombe and
P.M. Morris (1961, Monthly Not. Roy. Astron. Soc.  123, 233).


147)   HIP  30457 = FK 1171

   Radial velocity may be variable according to
T.G. Barnes et al. (1986, Publ. Astron. Soc. Pacific  98, 223).


148)   HIP  30520 = FK  242

   Radial velocity is variable according to BSC
and may be variable according to W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147).


149)   HIP  30678 = FK 1662

   Radial velocity may be variable according to J. Andersen and B. Nordstroem
(1983, Astron. Astrophys. Suppl. Ser. 52, 471).


150)   HIP  30772 = FK  246

   2 companions in CCDM+WDS:
B(1908:  77", 257 deg,  9.2 mag; nc, pc), C(1908:  81", 231 deg,  9.2 mag; nc, pc).
Radial velocity may be variable according to BSC.


151)   HIP  31278 = FK 1175

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


152)   HIP  31676 = FK  247

   3 companions in CCDM+WDS:
B(1923: 161",  79 deg,  9.1 mag; af), C(1904: 374",  95 deg,  7.0 mag; pc),
Q(BQ: 1907:  71", 253 deg, 12.8 mag; oo).


153)   HIP  31685 = FK  252

   Radial velocity is variable according to W.H. Wright (1911, Publ. Lick Obs.
9, 71) and D. Baade (1989, Astron. Astrophys. 222, 200).
Duplicity doubtful, mainly because of v_rot sin(i) = 225 km/s.


154)   HIP  31897 = FK  264

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


155)   HIP  32246 = FK  254

   1 companion in CCDM+WDS:
B(1982: 111",  94 deg,  9.2 mag; pc).
TYCHO gives for B(1991: 110",  95 deg,  9.64 mag). The proper
motions of A and B differ only slightly, but A is rather distant
(r_H = 277 pc). Radial velocity is variable according to BSC.


156)   HIP  32362 = FK  256

   Radial velocity may be variable according to BSC.


157)   HIP  32537 = FK 1178

   1 companion in CCDM+WDS:
B(1920:  65", 299 deg, 11.1 mag; nc:).


158)   HIP  32562 = FK 1176

   Radial velocity is variable according to BSC
and may be variable according to W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147).


159)   HIP  33018 = FK  261

   2 companions in CCDM+WDS:
B(1922:  78", 322 deg, 12.6 mag; ~oo), C(1922: 102", 185 deg, 12.7 mag; ~oo).
Radial velocity is variable according to BSC and WDS, but not to GCRV.


160)   HIP  33104 = FK  259

   Radial velocity may be variable according to BSC.


161)   HIP  33160 = FK  266

   Radial velocity may be variable according to BSC.


162)   HIP  33694 = FK  260

   Radial velocity is variable according to BSC.


163)   HIP  33977 = FK  270

   Radial velocity is variable according to BSC.


164)   HIP  34045 = FK  271

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


165)   HIP  34088 = FK  269

   4 companions in CCDM+WDS:
B(1984:  87",  84 deg, 10.5 mag; pc), C(1984: 100", 348 deg,  7.6 mag; pc),
P(1984:  70", 352 deg, 12.0 mag; pc), R(CR: 1908:  27", 166 deg, 12.9 mag; oo).
TYCHO gives for C(1991: 100", 348 deg, 7.58 mag).
Cepheid. The pulsation explains radial-velocity variations. T.S. Jacobsen and
G. Wallerstein (1982, Publ. Astron. Soc. Pacific  94, 471) conclude that
Zeta Gem is not a spectroscopic binary, since the gamma velocity of
the center-of-mass of the star has been
constant for 80 years. D.G. Turner and J. Fernie (1978, Inf. Bull. Variable
Stars No. 1509) investigate the possibility that the component B
(11.46 mag) is a physical companion of Zeta Gem. The separation of
87" between A and B corresponds to 0.16 pc at the distance of A.


166)   HIP  34387 = FK 1185

   Radial velocity may be variable according to BSC.


167)   HIP  34444 = FK  273

   Some older reports on radial-velocity variations (C. Payne, The Stars of High
Luminosity, New York and London, 1930, p. 302).
Radial velocity is constant according to W. Buscombe and P.M. Morris
(1961, Monthly Not. Roy. Astron. Soc.  123, 233).


168)   HIP  34752 = FK  274

   Radial velocity may be variable according to BSC.


169)   HIP  35228 = FK  281

   Radial velocity is possibly slightly variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


170)   HIP  35341 = FK  276

   Radial velocity is variable according to BSC.


171)   HIP  35904 = FK  283

   1 companion in CCDM+WDS:
B(1909: 179", 285 deg,  6.9 mag; nc, pc).
Radial velocity is variable according to BSC.


172)   HIP  35907 = FK 1191

   Radial velocity may be variable according to BSC.


173)   HIP  36046 = FK  282

   Radial velocity is variable according to BSC.


174)   HIP  36795 = FK  288

   1 companion in TYCHO:
B(1991:  83", 285 deg, 10.34 mag; oo).


175)   HIP  36942 = FK 1198

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


176)   HIP  37036 = FK 1197

   Radial velocity may be variable according to BSC. Beta Cephei star.


177)   HIP  37391 = FK  909

   Radial velocity is variable according to BSC.


178)   HIP  37891 = FK 1202

   Radial velocity is variable according to BSC.


179)   HIP  37921 = FK 1201

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


180)   HIP  37946 = FK 1199

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC.


181)   HIP  38373 = FK 1205

   Radial velocity may be variable according to BSC.


182)   HIP  38848 = FK 1208

   1 companion in TYCHO:
B(1991: 104", 168 deg, 10.44 mag; oo).


183)   HIP  39117 = FK  300

   Radial velocity may be variable according to BSC.


184)   HIP  39191 = FK 1211

   Radial velocity is variable according to BSC.


185)   HIP  39326 = FK 1213

   Radial velocity is variable according to BSC.


186)   HIP  39429 = FK  306

   Radial velocity may be variable according to BSC.


187)   HIP  40215 = FK 1215

   Radial velocity is variable according to BSC.


188)   HIP  40259 = FK  311

   Radial velocity may be variable according to BSC.


189)   HIP  40559 = FK 1639

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


190)   HIP  40793 = FK  310

   Radial velocity is variable according to BSC.


191)   HIP  40843 = FK 1217

   Radial velocity may be variable according to H.A. Abt and S.G. Levy (1976,
Astrophys. J. Suppl. Ser. 30, 273) and is probably variable according to
A. Duquennoy and M. Mayor (1991, Astron. Astrophys. 248, 485).


192)   HIP  41307 = FK  316

   Radial velocity is variable according to BSC.


193)   HIP  41578 = FK 1222

   The radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


194)   HIP  41935 = FK  320

   Radial velocity is variable according to BSC.


195)   HIP  42313 = FK 1223

   1 companion in CCDM+WDS:
B(1909: 244", 312 deg, 10.4 mag; nc).
Radial velocity is variable according to BSC and WDS.


196)   HIP  42452 = FK  323

   Radial velocity may be variable according to BSC.


197)   HIP  42484 = FK  322

   Radial velocity is variable according to BSC.


198)   HIP  42637 = FK  331

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


199)   HIP  42806 = FK 1228

   3 companions in CCDM+WDS:
B(1984: 112",  67 deg,  8.7 mag; nc), P(1908: 103", 258 deg, 12.4 mag; oo),
Q(BQ: 1908:  95", 102 deg, 12.9 mag; oo).
TYCHO gives for B(1991: 114",  66 deg, 10.20 mag).
Radial velocity is variable according to GCRV, BSC, WDS, and Sinzi (1972).


200)   HIP  42828 = FK  327

   2 companions in TYCHO:
B(1991: 107", 356 deg,  8.05 mag; oo), C(1991: 112", 151 deg, 10.78 mag; oo).
Radial velocity is variable according to C. Sterken and D. vander Linden (1983,
Inf. Bull. Variable Stars No. 2330).
They estimate a probable period of about 5 hours.


201)   HIP  43305 = FK 1230

   Radial velocity may be variable according to BSC.


202)   HIP  43798 = FK 1231

   1 companion in CCDM+WDS:
B(1918:  66", 146 deg,  7.1 mag; nc).
B is HIP 43800 (1991: 65", 150 deg, 7.06 mag; nc, hv).


203)   HIP  44356 = FK 1235

   Radial velocity is variable according to BSC.


204)   HIP  44382 = FK  343

   Radial velocity is variable according to GCRV and BSC.
Double-lined spectroscopic binary according to R.M. Catchpole et al.
(1982, Royal Obs. Bull. No. 188, 5).


205)   HIP  44390 = FK  338

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


206)   HIP  44504 = FK  340

   Radial velocity is variable according to BSC.


207)   HIP  44936 = FK 1240

   Radial velocity is variable according to BSC.


208)   HIP  45158 = FK 1242

   Radial velocity may be variable according to BSC.


209)   HIP  45238 = FK  348

   Radial velocity may be variable according to BSC.


210)   HIP  45290 = FK  346

   Radial velocity is variable according to BSC.


211)   HIP  45421 = FK 1640

   Radial velocity is variable (R.E. Wilson and A.H. Joy, 1952,
Astrophys. J. 115, 157; H.A. Abt, 1969, Astrophys. J. Suppl. Ser. 19, 387).
BSC gives SB2.


212)   HIP  45902 = FK 1243

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


213)   HIP  46221 = FK 1245

   1 companion in TYCHO:
B(1991:  74", 182 deg, 10.00 mag; oo).
Radial velocity is variable according to BSC.


214)   HIP  46390 = FK  354

   2 companions in CCDM+WDS:
B(1900: 284", 153 deg,  9.7 mag; nc),
C(1783: 210"; oo).
Radial velocity may be variable according to BSC.


215)   HIP  46515 = FK  356

   Radial velocity is variable according to BSC.


216)   HIP  46952 = FK  360

   Interferometric observations by P.W. Merrill (1922, Astrophys. J. 56, 40)
indicated possibly a binary star.
However, the object was not resolved by speckle observations
(H. McAlister, 1978, Publ. Astron. Soc. Pacific  90, 288;
W.I. Hartkopf and H.A. McAlister, 1984, Publ. Astron. Soc. Pacific  96, 105).


217)   HIP  47199 = FK 1248

   1 companion in TYCHO:
B(1991: 102",  93 deg,  8.92 mag; oo).


218)   HIP  47310 = FK 1249

   Radial velocity is variable according to BSC.


219)   HIP  47431 = FK 1250

   Radial velocity may be variable according to BSC.


220)   HIP  47452 = FK  364

   Radial velocity may be variable according to BSC.


221)   HIP  47594 = FK  363

   Radial velocity may be variable according to BSC.
HIP: goodness-of-fit parameter F2 = 4.03.


222)   HIP  47723 = FK 1252

   1 companion in CCDM+WDS:
B(1909: 282", 138 deg, 10.9 mag; pc).


223)   HIP  47854 = FK 1254

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Cepheid. This explains the observed radial-velocity variations.


224)   HIP  47908 = FK  367

   Radial velocity may be variable according to BSC.


225)   HIP  47909 = FK 1253

   Probably a spectroscopic binary according to D. Crampton and W. Morrison
(1979, Publ. Astron. Soc. Pacific  91, 695).


226)   HIP  48341 = FK  370

   Radial velocity is variable according to BSC.


227)   HIP  48615 = FK  373

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


228)   HIP  49339 = FK 1260

   Radial velocity is variable according to BSC.


229)   HIP  49402 = FK 1261

   Radial velocity is variable (O. Struve, 1925, Astrophys. J. 62, 434; R.
Woolley et al., 1981, Roy. Obs. Ann. No. 14, p. 5). BSC gives SB2.


230)   HIP  50099 = FK  385

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1960, Monthly. Not. Roy. Astron. Soc.  121, 263).


231)   HIP  50191 = FK  382

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


232)   HIP  50335 = FK  384

   1 companion in CCDM+WDS:
B(1925: 326", 340 deg,  5.9 mag; nc, pc).
B is HIP 50319 (1991: 332", 338 deg, 5.95 mag; nc, hv).
Radial velocity is variable according to Sinzi (1972), BSC, and WDS, but not to GCRV.
Barbier-Brossat (1989) gives v_rad = -20.6 km/s (Field 17: -15.6 km/s).


233)   HIP  50414 = FK 1263

   1 companion in TYCHO:
B(1991: 119", 230 deg, 11.15 mag; oo).
Radial velocity is variable according to BSC.


234)   HIP  50448 = FK 1262

   Radial velocity is variable according to BSC.


235)   HIP  50684 = FK 1266

   Radial velocity is variable according to BSC.
Beta Cephei star. The pulsation explains the radial-velocity variations.


236)   HIP  50860 = FK 1267

   Radial velocity is variable according to BSC.


237)   HIP  50954 = FK  391

   Radial velocity is variable according to GCRV and BSC.
D.S. Evans et al. (1959, Monthly Not. Roy. Astron. Soc.  119, 638) doubt this.


238)   HIP  51172 = FK  392

   Radial velocity is variable according to BSC.


239)   HIP  51362 = FK 1270

   Radial velocity is variable according to BSC.


240)   HIP  51399 = FK 1271

   1 companion in CCDM+WDS:
B(1924: 131", 226 deg,  8.3 mag; nc, pc).
B is HIP 51390 (1991: 134", 226 deg, 8.10 mag; nc, hv).


241)   HIP  51585 = FK 1272

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to BSC.


242)   HIP  51814 = FK  398

   Radial velocity is variable according to BSC.


243)   HIP  52098 = FK 1275

   Radial velocity is variable according to BSC.


244)   HIP  52316 = FK  404

   Radial velocity may be variable according to BSC.


245)   HIP  52457 = FK  405

   Radial velocity is variable according to BSC.


246)   HIP  52638 = FK  407

   1 companion in CCDM+WDS:
B(1960: 198", 174 deg,  8.2 mag; nc, pc).
B is HIP 52645 (1991: 197", 173 deg, 7.64 mag; nc, hv).
Radial velocity is variable according to BSC.


247)   HIP  52660 = FK 1278

   Radial velocity is variable according to BSC.


248)   HIP  52911 = FK  409

   Radial velocity is variable ccording to BSC.


249)   HIP  53229 = FK  412

   Radial velocity is variable ccording to BSC.


250)   HIP  53702 = FK 1664

   1 companion in TYCHO:
B(1991: 115", 34 deg, 10.25 mag; oo).


251)   HIP  53721 = FK 1282

   The star has a planetary companion
(R.P. Butler and G.W. Marcy, 1996, Astrophys. J. 464, L153).


252)   HIP  53761 = FK  413

   Radial velocity may be variable according to BSC.


253)   HIP  53910 = FK  416

   Radial velocity is variable according to BSC.


254)   HIP  54463 = FK 1289

   Radial-velocity variations may be due to a Cepheid-like pulsation of this
yellow supergiant V382 Car (L.A. Ballona, 1982, Monthly Not. Roy.
Astron. Soc.  201, 105).


255)   HIP  54725 = FK 1290

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


256)   HIP  54872 = FK  422

   2 companions in CCDM+WDS:
B(1924: 191", 344 deg,  8.6 mag; nc), P(1911:  95",  41 deg, 12.1 mag; nc).
Radial velocity is variable according to BSC.


257)   HIP  54879 = FK  423

   Radial velocity is variable according to BSC.


258)   HIP  55084 = FK 1292

   1 companion in CCDM+WDS:
B(1923:  97", 289 deg,  8.5 mag; nc).
TYCHO gives for B(1991:  89", 290 deg,  9.75 mag).
Radial velocity is variable according to Sinzi (1972) or may be variable according
to BSC, but not to GCRV.


259)   HIP  55086 = FK  424

   Radial velocity may be variable according to BSC.


260)   HIP  55282 = FK  426

   Radial velocity is variable according to BSC.


261)   HIP  55434 = FK  427

   Radial velocity is variable according to BSC.


262)   HIP  55781 = FK 1295

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


263)   HIP  55945 = FK 1297

   3 companions in CCDM+WDS:
B(1985:  90", 180 deg,  8.1 mag; nc), C(BC: 1910: 107", 234 deg, 14.4 mag; pc),
D(1875: 765",  92 deg, 10.0 mag; pc).
TYCHO gives for B(1991:  89", 180 deg, 7.42 mag).


264)   HIP  56343 = FK  434

   1 companion in CCDM+WDS:
B(1928:  68", 149 deg, 10.7 mag; af).
Radial velocity is variable according to BSC.


265)   HIP  56633 = FK 1299

   Radial velocity is variable according to BSC.


266)   HIP  56997 = FK 1300

   1 companion in CCDM+WDS:
B(1925: 158",  98 deg, 10.4 mag; af).
Radial velocity is variable according to BSC.


267)   HIP  57111 = FK  440

   Radial velocity may be variable according to BSC.


268)   HIP  57380 = FK 1302

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to BSC.


269)   HIP  57399 = FK  441

   Radial velocity is variable according to BSC.


270)   HIP  57613 = FK 1305

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


271)   HIP  57757 = FK  445

   2 companions in CCDM+WDS:
B(1984: 305", 285 deg, 10.6 mag; af), C(1884: 512",  85 deg,  8.8 mag; oo).
The absolute proper motions of A and C differ significantly. Radial velocity is
constant according to G.A.H. Walker et al. (1995, Icarus  116, 359).


272)   HIP  57939 = FK 1307

   P. van de Kamp (1968, in: Low Luminosity Stars. Ed. S. Kumar. Gordon and
Breach, New York, p. 199) reported a companion with a separation of
rho ~1.7" on parallax plates.
He considered the rarely seen companion to be a flare star.
In 1968, C. Worley and W.D. Heintz carried out visual observations
and noticed a companion with rho ~2". W.R. Beardsley et al. (1974,
Astrophys. J. 194, 637) found evidence for orbital motion from
radial-velocity variations and positional displacements on parallax plates.
They obtained an orbital period of P = 60 years. R.F. Griffin (1984,
Observatory  104, 192) did not confirm significant variations in the
radial velocity. In a rediscussion of the binary nature of the object, W.D.
Heintz (1984, Publ. Astron. Soc. Pacific  96, 557) concluded that no
evidence for orbital effects of the unconfirmed visual companion is found in
the astrometric observations.
The very high value of F_0(GC)H of 9.06 should not be taken as a firm
confirmation of the binary nature of the object. Firstly, the proper-motion
differences from the FK5/HIP comparison give much smaller values of F: The
highest value is F_0F = 3.53, while the usually most sensitive quantity
F_FH = 1.93 is not significantly different from a value expected for a
single star. Secondly, F_0(GC)H is probably affected by an incorrect
treatment of the foreshortening effect for this nearby high-proper motion star
in the GC. This is indicated by the fact that the vector of
Delta_mu_0(GC)H is anti-parallel to the vector of mu within a tolerance
of less than 0.6 degrees. Such a nearly perfect alignment of
Delta_mu and mu would be extremely improbable for a Delta_mu binary,
but is fully consistent with a slight error in the foreshortening treatment in
the GC, in which case we expect that Delta_mu is parallel or anti-parallel
to mu.


273)   HIP  58001 = FK  447

   Probably not a spectroscopic binary according to S. Hubrig and G. Mathys
(1994, Astron. Nachr.  315, 347).


274)   HIP  58188 = FK 1309

   Radial velocity may be variable according to BSC.


275)   HIP  58874 = FK 1642

   Radial velocity may be variable according to BSC.


276)   HIP  58948 = FK  450

   Radial velocity may be variable according to BSC.


277)   HIP  58952 = FK  451

   Radial velocity is variable according to BSC.


278)   HIP  59747 = FK  455

   Radial velocity may be variable according to BSC.


279)   HIP  59774 = FK  456

   2 companions in CCDM+WDS:
B(1923: 189",  73 deg, 10.0 mag; af), C(1907: 186", 125 deg, 11.6 mag; af).
Radial velocity is variable according to BSC.
Beta Cephei star. The pulsation explains the radial-velocity variations.


280)   HIP  59803 = FK  457

   Radial velocity is variable according to BSC.


281)   HIP  60122 = FK 1316

   Radial velocity is variable according to BSC.


282)   HIP  60172 = FK 1317

   1 companion in CCDM+WDS:
B(1925: 132",   4 deg, 11.6 mag; nc).
Radial velocity may be variable according to BSC.


283)   HIP  60646 = FK  461

   Radial velocity may be variable according to BSC.


284)   HIP  60823 = FK  464

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


285)   HIP  60957 = FK  466

   Double-lined spectroscopic binary according to G. Hill et al. (1976, Mem.
Roy. Astron. Soc.  82, 69).


286)   HIP  61084 = FK  468

   2 companions in CCDM+WDS:
B(1919: 111",  31 deg,  6.4 mag; af), C(1880: 155",  82 deg,  9.5 mag; oo).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


287)   HIP  61199 = FK  469

   Radial velocity may be variable according to BSC.
HIP: goodness-of-fit parameter F2 = 3.29.


288)   HIP  61296 = FK 1321

   Radial velocity may be variable according to BSC.


289)   HIP  61309 = FK 1322

   Radial velocity is variable according to BSC.


290)   HIP  61558 = FK 1324

   Radial velocity is variable according to BSC.


291)   HIP  61740 = FK  475

   3 companions in CCDM+WDS:
B(1924: 174", 137 deg,  9.1 mag; nc), C(1924: 223", 110 deg, 10.4 mag; nc, pc),
D(1924: 321", 331 deg,  9.1 mag; pc).
D is HIP 61721 (1991: 321", 331 deg, 8.93 mag; nc, hv).


292)   HIP  61916 = FK 1325

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


293)   HIP  61960 = FK 1326

   Radial velocity may be variable (e.g.: R.O. Gray, 1988, Astron. J.  95,
220). It is a Lambda Bootis star with v_rot sin(i) ~175 km/s.
Not necessarily a spectroscopic binary.


294)   HIP  62131 = FK  479

   Radial velocity is variable according to BSC.


295)   HIP  62223 = FK 1327

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is slightly variable. This may be due to pulsation rather than
to duplicity (C. Barnbaum and K.H. Hinkle, 1995, Astron. J.  110, 805).


296)   HIP  62443 = FK 1330

   Radial velocity may be variable according to BSC.


297)   HIP  62448 = FK 1329

   Radial velocity is variable according to BSC.


298)   HIP  62763 = FK 1332

   Radial velocity may be variable according to BSC.


299)   HIP  62807 = FK 1333

   2 companions in CCDM+WDS:
B(1960: 196",  51 deg,  6.9 mag; nc, pc), C(1910: 897", 262 deg,  8.9 mag; pc).
B is HIP 62819 (1991: 196", 51 deg, 6.93 mag; nc, hv).
C is HIP 62718 (1991: 905", 262 deg, 8.78 mag; nc, hv).
Radial velocity may be variable according to BSC.


300)   HIP  62985 = FK 1335

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


301)   HIP  63090 = FK  484

   1 companion in CCDM+WDS:
B(1925: 165", 138 deg, 10.7 mag; af).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147).


302)   HIP  63608 = FK  488

   1 companion in CCDM+WDS:
B(1909: 249", 120 deg, 11.9 mag; nc).


303)   HIP  63901 = FK 1337

   Radial velocity is variable according to BSC.


304)   HIP  64246 = FK  491

   2 companions in CCDM+WDS:
B(1922: 284", 297 deg,  6.3 mag), C(BC: 1991:   1", 271 deg,  9.5 mag).
B is HIP 64217 (279", 297 deg,  6.25 mag; nc, hv).
Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity.
Radial velocity may be variable, and the object shows probably a composite
spectrum (G. Hill et al., 1976, Memoirs Roy. Astron. Soc.  82, 69).
Barbier-Brossat (1989) gives v_rad = -16.4 km/s (Field 17: 0.0 km/s).


305)   HIP  64394 = FK  492

   1 companion in CCDM+WDS:
B(1924:  86", 238 deg, 10.1 mag; af).
Radial velocity was supposed to be variable with a possible period of 5 years or
more by H.A. Abt and S.G. Levy (1976, Astrophys. J. Suppl. Ser. 30, 273).
Radial velocity is constant  according to G.A.H. Walker et al.
(1995, Icarus  116, 359).


306)   HIP  64803 = FK 1342

   Radial velocity may be variable according to BSC.


307)   HIP  64844 = FK  494

   Delta Scuti star FM Vir.
The radial-velocity variations are probably caused by pulsation
(e.g. S. Yang and G.A.H. Walker, 1986, Publ. Astron. Soc. Pacific 98, 862).


308)   HIP  64852 = FK 1344

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to BSC.


309)   HIP  64924 = FK 1345

   1 companion in CCDM+WDS:
B(1907: 232",  29 deg, 10.3 mag; af).
Radial velocity is possibly variable according to according to B. Campbell et al.
(1988, Astrophys. J. 331, 902) and is constant according to
G.A.H. Walker et al. (1995, Icarus  116, 359).


310)   HIP  64962 = FK  495

   1 companion in CCDM+WDS:
B(1891: 138",  97 deg, 10. mag; nc).
Radial velocity may be variable according to BSC.


311)   HIP  65581 = FK 1348

   Radial velocity may be variable according to BSC.


312)   HIP  65721 = FK 1349

   2 companions in CCDM+WDS:
B(1923: 285", 136 deg,  8.8 mag; nc), C(1923: 326", 263 deg; oo).
B is HIP 65749 (1991: 270", 127 deg,  8.58 mag; nc, hv).
The star has a planetary companion (G.W. Marcy and R.P. Butler,
1996, Astrophys. J. 464, L147).


313)   HIP  66200 = FK 1351

   Radial velocity is variable according to BSC.


314)   HIP  66607 = FK  503

   Double-lined spectroscopic binary according to J. Andersen and B. Nordstroem
(1977, Astron. Astrophys. Suppl. Ser. 29, 309).


315)   HIP  66753 = FK 1665

   Radial velocity is variable according to F.J. Neubauer (1930, Lick Obs.
 Bull. 15, 47).


316)   HIP  66803 = FK 1355

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


317)   HIP  66878 = FK 1643

   Radial velocity is variable according to BSC.


318)   HIP  66925 = FK 1356

   1 companion in TYCHO:
B(1991:  88",  30 deg, 10.22 mag; pc).
Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


319)   HIP  67057 = FK 1357

   Radial velocity is variable according to BSC.


320)   HIP  67301 = FK  509

   Spectroscopic binary according to K. Kodaira (1971, Publ. Astron. Soc. Japan
23, 159) with a period of P = 289.13 days. Not confirmed by H.A.
Abt and S.G. Levy (1978, Astrophys. J. Suppl. Ser. 36, 241).


321)   HIP  67481 = FK 1359

   Radial velocity is possibly variable according to
A.H. Batten (1976, Publ. Dominion Astrophys. Obs. 14, 367).


322)   HIP  68269 = FK  515

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


323)   HIP  68390 = FK 1361

   Radial velocity may be variable according to BSC.


324)   HIP  68478 = FK  517

   Radial velocity is variable according to BSC.


325)   HIP  68520 = FK  516

   2 companions in CCDM+WDS:
B(1961:  81", 290 deg,  9.5 mag; nc), C(1960: 177", 353 deg, 12.5 mag; oo).
Radial velocity is variable according to BSC and WDS, but not to GCRV.


326)   HIP  68673 = FK 1364

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


327)   HIP  68763 = FK 1365

   1 companion in TYCHO:
B(1991: 102", 348 deg,  9.78 mag; oo).
Radial velocity is variable according to W. Buscombe and P.M. Morris
(1961, Monthly Not. Roy. Astron. Soc.  123, 233).


328)   HIP  68933 = FK  520

   1 companion in CCDM+WDS:
B(1897:  70", 129 deg, 14.3 mag; oo).
A faint companion (m ~8.0) with a separation of rho ~3", seen
by J. Dunlop in 1826 and by the Harvard observers at Arequipa in 1891, is
probably not real (R.T.A. Innes and D. Gill, 1899, Ann. Cape Obs.  2,
part II; T.J.J. See, 1898, Astron. J.  18, 181).


329)   HIP  69038 = FK 1368

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


330)   HIP  69701 = FK  525

   Deviations from a linear motion of the star as an indication for duplicity
have been noted by H. Schwan during the construction of the FK5
and by L.V. Morrison et al. (1990, Astron. Astrophys. 240, 173)
in a comparison of recent meridian-circle positions with the FK5 prediction.


331)   HIP  69989 = FK 1372

   1 companion in CCDM+WDS:
B(1922: 157", 217 deg, 10.2 mag; nc).
Radial velocity may be variable according to BSC.


332)   HIP  70069 = FK  529

   Radial velocity may be variable according to BSC.


333)   HIP  70400 = FK 1375

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


334)   HIP  70469 = FK 1376

   Radial velocity may be variable according to BSC.


335)   HIP  70492 = FK  530

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


336)   HIP  70574 = FK 1377

   1 companion in CCDM+WDS:
B(1913: 158", 204 deg,  9.3 mag; nc, pc).


337)   HIP  71040 = FK  536

   Radial velocity may be variable according to BSC.


338)   HIP  71284 = FK 1380

   2 companions in CCDM+WDS:
B(1924: 233",  83 deg,  9.8 mag; nc), C(1907: 237",  97 deg, 11.3 mag; af).
Radial velocity is probably variable according to A. Duquennoy and M. Mayor
(1991, Astron. Astrophys. 248, 485).


339)   HIP  71352 = FK  537

   Probably an eclipsing binary according to HIP. Composite spectrum and
radial-velocity variations suggested a spectroscopic-binary nature of this
object (e.g.: W.H. Wright, 1909, Lick Obs. Bull.  5, 176; A.J. Cannon and
E.C. Pickering, 1920, Annals Astron. Obs. Harvard Coll.  95, especially p.
313). J. Dachs et al.
(1986, Astron. Astrophys. Suppl. Ser. 63, 87) argue that
the binary appearance is spurious and caused by other effects (Be-shell star).
S. Stefl et al. (1995, Astron. Astrophys. 294, 135) conclude that the available
data cannot exclude a contact binary with an 0.6-day orbital period.
v_rot sin(i) ~ 350 km/s.
T.J.J. See (1898, Astron. J.  18, 181) reported three observations of a
visual companion in 1897 with rho ~6" and  m_B ~14.8. No further
observations are available. The object is removed
from modern double-star catalogues (such
as the WDS). Sinzi (1972) mentions a common-proper-motion companion, which we
could not identify. Probably he had in mind the companion announced by See.


340)   HIP  71618 = FK  540

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


341)   HIP  71837 = FK 1382

   Radial velocity is variable according to BSC.


342)   HIP  71957 = FK  545

   Radial velocity is variable (W.W. Campbell, 1913, Lick Obs. Bull.  7, 113;
H.A. Abt and S.G. Levy, 1976, Astrophys. J. Suppl. Ser. 30, 273).
Abt and Levy (1976) give a probable orbital period of P ~358 days.


343)   HIP  71995 = FK 1383

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to W.I. Beavers and J.J. Eitter
(1986, Astrophys. J. Suppl. Ser. 62, 147).


344)   HIP  72124 = FK 1384

   Radial velocity is variable according to BSC.


345)   HIP  72220 = FK  547

   Radial velocity may be variable according to BSC.


346)   HIP  72469 = FK 1386

   Radial velocity may be variable according to BSC.


347)   HIP  72573 = FK 1644

   Radial velocity is variable according to BSC.


348)   HIP  72607 = FK  550

   1 companion in CCDM+WDS:
B(1908: 209", 342 deg, 11.4 mag; nc).
Radial velocity is variable according to BSC.


349)   HIP  72664 = FK  549

   Radial velocity may be variable according to BSC.


350)   HIP  73087 = FK  551

   Radial velocity may be variable according to BSC.


351)   HIP  73133 = FK 1390

   Radial velocity is variable according to BSC.


352)   HIP  73273 = FK  552

   Radial velocity is variable according to H. Levato et al. (1987,
Astrophys. J. Suppl. Ser. 64, 487).


353)   HIP  73714 = FK  556

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


354)   HIP  73909 = FK 1397

   Radial velocity may be variable according to BSC.


355)   HIP  73996 = FK 1396

   2 companions in CCDM+WDS:
B(1923: 106",  51 deg, 10.8 mag; nc), C(1923: 243",  40 deg,  9.9 mag; nc).
Radial velocity is variable according to BSC.


356)   HIP  74785 = FK  564

   Radial velocity may be variable (D.B. McLaughlin, 1932, Publ. Obs. Univ.
Michigan, Vol. IV, No. 2, p. 29).
W. Buscombe and P.M. Kennedy (1965, Monthly Not. Royal Astron. Soc.  130, 281)
list Beta Lib under stars with constant radial velocities.


357)   HIP  74946 = FK  560

   Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


358)   HIP  75097 = FK  569

   Delta Scuti star.
O. Struve (1923, Popular Astron. 31, 90) presented a spectroscopic-binary orbit
for gamma UMi with an orbital period of about 0.11 days. This orbit is
probably spurious. The radial-velocity variations are more probably due to
pulsations or shell effects (e.g. H.F. Weaver, 1952, Astrophys. J. 116, 541).


359)   HIP  75304 = FK 1403

   Radial velocity is variable according to H. Levato et al. (1987,
Astrophys. J. Suppl. Ser. 64, 487).


360)   HIP  75342 = FK 1406

   Radial velocity is variable according to BSC.


361)   HIP  75458 = FK  571

   1 companion in CCDM+WDS:
B(1909: 255",  50 deg,  9.2 mag; unclear).
Separation rho corresponds to 0.04 pc, if A and B are at a common distance.


362)   HIP  75730 = FK 1407

   Radial velocity may be variable according to BSC.


363)   HIP  76440 = FK  574

   1 companion in CCDM+WDS:
B(1918:  83", 218 deg,  9.5 mag; nc:).
TYCHO gives for B(1991:  82", 220 deg,  9.32 mag).
Radial velocity may be variable according to BSC.


364)   HIP  76534 = FK  580

   Radial velocity may be variable according to BSC.


365)   HIP  76996 = FK 1666

   1 companion in TYCHO:
B(1991:  66", 333 deg, 10.55 mag; oo).


366)   HIP  77055 = FK  590

   Radial velocity is variable according to BSC.


367)   HIP  77277 = FK  587

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


368)   HIP  77622 = FK  588

   Radial velocity is variable according to BSC.


369)   HIP  77655 = FK 1414

   1 companion in CCDM+WDS:
B(1926: 135", 203 deg, 11.5 mag; nc).


370)   HIP  78072 = FK  591

   2 companions in CCDM+WDS:
B(1924: 220", 318 deg, 10.5 mag; af), C(BC: 1908: 177", 165 deg, 10.9 mag; oo).
The separation of AC was 101" in 1908.
Radial velocity may be variable according to BSC.


371)   HIP  78180 = FK  595

   Radial velocity is variable according to BSC.
Delta Scuti star CL Dra. The pulsation explains the radial-velocity variations.


372)   HIP  78207 = FK 1417

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.
v_rot sin(i) ~400 km/s (R.W. Hanuschik, 1986, Astron.
Astrophys. 166, 185).


373)   HIP  78436 = FK 1420

   Radial velocity may be variable according to P.C. Frisch (1987, Astrophys. J.
Suppl. Ser.  65, 313).


374)   HIP  79137 = FK 1422

   Radial velocity is variable according to BSC.


375)   HIP  79280 = FK  606

   Radial velocity is variable according to BSC.


376)   HIP  79593 = FK  603

   2 companions in CCDM+WDS:
B(1908:  66", 295 deg, 13.4 mag; nc), C(1879: 266", 127 deg, 10.0 mag; oo).
Radial velocity is variable according to BSC.
and may be variable according to T.G. Barnes et al. (1986,
Publ. Astron. Soc. Pacific  98, 223).
HIP: percentage of rejected data F1 = 4%.


377)   HIP  80047 = FK 1424

   2 companions in CCDM+WDS:
B(1919: 103",  12 deg,  5.3 mag; pc), C(1919:  90",  74 deg, 12.5 mag; pc).
B is HIP 80057 (1991: 103",  10 deg,  5.27 mag; hv).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


378)   HIP  80179 = FK 1427

   Radial velocity may be variable according to BSC.


379)   HIP  80375 = FK  614

   1 companion in TYCHO:
B(1991:  85", 116 deg,  9.60 mag; oo).
HIP: percentage of rejected data F1 = 4%.


380)   HIP  80650 = FK  619

   Radial velocity is variable according to BSC.


381)   HIP  80850 = FK  623

   Radial velocity may be variable according to BSC.


382)   HIP  80911 = FK 1431

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.


383)   HIP  80991 = FK 1432

   Radial velocity is variable according to BSC.


384)   HIP  81065 = FK  611

   In contrast to earlier claims (e.g., W.H. Wright, 1911, Publ. Lick Obs.
9, 71), the radial velocity does not seem to be variable (K.A. Murdoch et
al., 1993, Astrophys. J. 413, 349).


385)   HIP  81266 = FK  620

   Radial velocity is variable
according to Sinzi (1972) and BSC, but not to GCRV.
Radial velocity may be variable according to
H. Levato et al. (1987, Astrophys. J. Suppl. Ser. 64, 487).


386)   HIP  81300 = FK 1433

   1 companion in CCDM+WDS:
B(1910: 100", 245 deg, 13.4 mag; oo).
Radial velocity may be variable or constant
according to A. Young et al. (1987, Astrophys. J. 317, 787).


387)   HIP  81377 = FK  622

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1960, Monthly Not. Roy. Astron. Soc.  121, 263)
and may be variable according to P.S. Conti et al. (1977, Astrophys. J. 214, 759).
Barbier-Brossat (1989) gives v_rad = -9 km/s (Field 17: -15 km/s).


388)   HIP  81833 = FK  626

   2 companions in CCDM+WDS:
B(1901: 114", 262 deg, 12. mag; unclear), P(1879:  80", 260 deg; oo).
Radial velocity may be variable according to BSC.


389)   HIP  82351 = FK 1437

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


390)   HIP  82526 = FK  629

   Radial velocity may be variable according to BSC.


391)   HIP  82587 = FK 1441

   1 companion in CCDM+WDS:
B(1961:  71",  64 deg, 12.1 mag; af).


392)   HIP  82673 = FK 1442

   Radial velocity is variable (e.g.: W.W. Campbell, 1910, Lick Obs. Bull.
6, 57; R. Woolley et al., 1981, Roy. Obs. Ann. No. 14, p. 5). Lick Observatory
reports spectra of two stars, but later observations do not confirm this.


393)   HIP  83057 = FK 1444

   Radial velocity is variable according to BSC.


394)   HIP  83153 = FK  632

   Sinzi (1972) indicates a common-proper-motion companion. We were unable
to identify such a star.


395)   HIP  83262 = FK 1445

   1 companion in CCDM+WDS:
B(1923:  94",  69 deg,  9.8 mag; nc?).
TYCHO gives for B(1991:  99",  68 deg,  9.64 mag).
Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity.


396)   HIP  83313 = FK 1446

   Radial velocity may be variable according to BSC.


397)   HIP  83593 = FK 1448

   Flag D in HIP Field H52, based on HIP photometry. This could be an indication
of duplicity.


398)   HIP  83613 = FK  635

   1 companion in CCDM+WDS:
B(1924:  56", 309 deg, 10.9 mag; af).
INCA gives B( 60", 307 deg, 10.9 mag).
At present, the separation is probably slightly larger than 60".
Radial velocity may be variable according to BSC.


399)   HIP  83740 = FK 1447

   1 companion in TYCHO:
B(1991: 112", 123 deg, 10.46; pc).
Radial velocity is variable according to BSC.


400)   HIP  83854 = FK 1449

   Radial velocity may be variable according to BSC.


401)   HIP  83962 = FK 1450

   Radial velocity may be variable according to BSC.


402)   HIP  84862 = FK 1456

   2 companions in CCDM+WDS:
B(1983: 289", 338 deg,  9.7 mag; af), C(BC: 1911:   9", 216 deg, 12.9 mag).
Radial velocity is variable according to BSC.
and may be variable according to T.G. Barnes et al. (1986,
Publ. Astron. Soc. Pacific  98, 223).


403)   HIP  85379 = FK  650

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


404)   HIP  85696 = FK  649

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


405)   HIP  85760 = FK 1455

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


406)   HIP  85805 = FK  659

   1 companion in CCDM+WDS:
B(1960: 103", 344 deg, 11.4 mag; nc:).
Radial velocity is variable according to GCRV, Sinzi (1972), BSC, and WDS.


407)   HIP  85822 = FK  913

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to BSC.


408)   HIP  85888 = FK 1462

   Radial velocity may be variable according to BSC.


409)   HIP  86670 = FK  660

   Beta Cephei star.
Radial velocity is variable (N.R. Lomb and R.R. Shobrook, 1975, Monthly Not.
Roy. Astron. Soc.  173, 709). This may be due to pulsation (J.R. King and
T. Liu, 1990, Publ. Astron. Soc. Pacific  102, 328).


410)   HIP  86736 = FK 1463

   BSC classifies the star as a double star with a separation of  0.02" and
a magnitude difference of 1.8, but remarks that the duplicity is uncertain.


411)   HIP  86742 = FK  665

   Radial velocity is variable according to BSC.


412)   HIP  87072 = FK 1464

   Cepheid X Sgr. This explains the observed radial-velocity variations.


413)   HIP  87108 = FK  668

   Proposed as spectroscopic binary by O.J. Lee (1910, Astrophys. J. 32,
300). Duplicity very uncertain according to E.B. Frost et al. (1929, Publ.
Yerkes Obs.  7, 1).


414)   HIP  87234 = FK  675

   1 companion in TYCHO:
B(1991: 111",  57 deg, 10.50 mag; oo).


415)   HIP  87289 = FK 1466

   Radial velocity may be variable according to J. Andersen and B. Nordstroem
(1983, Astron. Astrophys. Suppl. Ser. 52, 479).


416)   HIP  87585 = FK  671

   1 companion in CCDM+WDS:
B(1963: 316", 290 deg, 15.6 mag; oo).
Radial velocity may be variable according to BSC.


417)   HIP  88258 = FK 1470

   1 companion in TYCHO:
B(1991:  72", 222 deg, 11.19 mag; pc).
Radial velocity may be variable according to BSC.


418)   HIP  88635 = FK  679

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


419)   HIP  89482 = FK  684

   Radial velocity is variable according to BSC.


420)   HIP  89605 = FK 1474

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


421)   HIP  89962 = FK  688

   1 companion in CCDM+WDS:
B(1924: 180",  61 deg, 12.1 mag; af).
Radial velocity may be variable according to BSC.


422)   HIP  90139 = FK  690

   2 companions in CCDM+WDS:
B(1924: 226", 321 deg, 10.4 mag; af), P(1924: 145",  91 deg; oo).
Radial velocity may be variable according to BSC.


423)   HIP  90422 = FK  691

   Radial velocity may be variable according to BSC.


424)   HIP  90496 = FK  692

   1 companion in TYCHO:
B(1991:  88", 186 deg,  9.84 mag; oo).


425)   HIP  90595 = FK  696

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.


426)   HIP  90642 = FK 1480

   W.H. Christie (1933, Publ. Astron. Soc. Pacific  45, 190)
presented a set of preliminary orbital elements
for 60 Ser as a spectroscopic binary. H.A. Abt and S.G. Levy  (1971,
Publ. Astron. Soc. Pacific  83, 687) found no convincing evidence
for the duplicity of this object.


427)   HIP  90647 = FK  700

   Radial velocity may be variable according to BSC.


428)   HIP  90762 = FK 1481

   Radial velocity may be variable according to BSC.


429)   HIP  90982 = FK  697

   Radial velocity is variable according to Sinzi (1972) or may be
variable according to BSC, but not to GCRV.


430)   HIP  91262 = FK  699

   4 companions in CCDM+WDS:
B(1947:  63", 173 deg,  9.5 mag; af), C(1899:  54", 285 deg, 11.0 mag; nc:),
D(CD: 1897:  31",  35 deg; oo), E(1922: 118",  39 deg,  9.5 mag; nc).
Present separation between A and C and between A and D probably larger than 60".
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC. Delta Scuti star.


431)   HIP  92041 = FK 1487

   Radial velocity may be variable (O.J. Lee, 1910, Astrophys. J. 32, 300;
W.W. Campbell and J.H. Moore, 1928, Lick. Obs. Bull.  16, 273). Probably
indications for binarity during lunar occultations (1929-1933). R.H. Wilson
(1950, Astron. J.  55, 153 and 1951, Astron. J.  56, 69) reported
duplicity with rho ~0.2". The visual-binary nature was found to
be spurious by W.H. van den Bos (1951, Journal des Obs.  34, 85) and by
W.S. Finsen (1951, Astron. J.  56, 56).


432)   HIP  92088 = FK 1488

   Radial velocity may be variable according to BSC.


433)   HIP  92609 = FK  704

   1 companion in CCDM+WDS:
B(1918:  63", 206 deg, 12.4 mag; pc).
Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


434)   HIP  92855 = FK  706

   1 companion in CCDM+WDS:
B(1838: 309", 244 deg,  9.5 mag; pc).
Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


435)   HIP  92862 = FK  711

   Semi-regular variable star R Lyr.
Radial velocity is variable.
Formerly interpreted as a triple stellar system (BSC).
In reality, the radial-velocity variations are most probably due to pulsation
(V.C. Cristian et al., 1995, Publ. Astron. Soc. Pacific  107, 411;
F. Kerschbaum et al., 1996, Astron. Astrophys. 311, 273).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


436)   HIP  92882 = FK 1495

   1 companion in TYCHO:
B(1991:  67", 111 deg,  9.53 mag; oo).
Radial velocity may be variable according to BSC.


437)   HIP  93148 = FK  708

   Radial velocity is variable according to GCRV and W. Buscombe and P.M.
Morris (1958, Monthly Not. Roy. Astron. Soc.  118, 609).


438)   HIP  93805 = FK  717

   Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


439)   HIP  93843 = FK 1498

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


440)   HIP  94376 = FK  723

   1 companion in CCDM+WDS:
B(1907:  88", 352 deg, 12.4 mag; nc).


441)   HIP  94385 = FK 1500

   Radial velocity is probably variable according to
H.A. Abt et al. (1990, Astrophys. J. Suppl. Ser. 74, 551).


442)   HIP  94713 = FK  724

   2 companions in CCDM+WDS:
B(1964: 100",  74 deg,  9.2 mag; nc, pc), C(1908: 101", 127 deg, 11.0 mag; pc).
TYCHO gives for B(1991:  99",  70 deg, 10.14 mag).


443)   HIP  94714 = FK 1499

   Radial velocity is variable according to
B. Nordstroem and J. Andersen (1985, Astron. Astrophys. Suppl. Ser. 61, 53).


444)   HIP  94779 = FK  726

   Radial velocity is variable according to BSC.


445)   HIP  94834 = FK  725

   Radial velocity is variable according to BSC.
HIP: percentage of rejected data F1 = 4%.


446)   HIP  94986 = FK 1501

   Radial velocity is variable
according to W. Buscombe (1963, Monthly Not. Roy. Astron. Soc.  126, 29).


447)   HIP  95167 = FK  734

   1 companion in TYCHO:
B(1991: 110", 182 deg, 10.48 mag; oo).
Radial velocity is variable according to BSC.


448)   HIP  95347 = FK  728

   Radial velocity is variable according to GCRV and to
W. Buscombe (1963, Monthly Not. Roy. Astron. Soc.  126, 29).


449)   HIP  95447 = FK 1503

   2 companions in CCDM+WDS:
B(1926:  99", 335 deg,  8.7 mag; af), C(1922: 114", 316 deg, 10.6 mag; af).
TYCHO gives for B(1991:  96", 295 deg,  8.55 mag).
Radial velocity is probably variable according to A. Duquennoy and M. Mayor
(1991, Astron. Astrophys. 248, 485).


450)   HIP  95619 = FK  731

   Radial velocity may be variable according to BSC.


451)   HIP  95690 = FK 1504

   3 companions in CCDM+WDS:
B(1985:  74", 240 deg,  8.3 mag; nc), C(BC: 1932: 8", 195 deg, 12.8 mag; nc),
D(1873:  71",  96 deg, 11. mag; oo).
TYCHO gives for B(1991:  74", 239 deg, 8.32 mag) and D(1991: 10.76 mag).
BSC claims a common proper motion of A and B. This is unjustified, since B is
a high-proper motion star (LTT 7685), while A has a small proper motion.


452)   HIP  95771 = FK 1508

   1 companion in CCDM+WDS:
B(1925: 414",  28 deg,  5.8 mag; af).
B is HIP 95785 (1991: 423", 28 deg,  5.82 mag; nc, hv).
Radial velocity may be variable according to BSC.


453)   HIP  95853 = FK  733

   Radial velocity may be variable according to BSC.


454)   HIP  95937 = FK 1509

   Radial velocity may be variable according to BSC.


455)   HIP  96052 = FK 1510

   1 companion in TYCHO:
B(1991: 116", 203 deg, 10.90 mag; pc).
Radial velocity may be variable according to BSC.


456)   HIP  96483 = FK  737

   Radial velocity is variable according to Sinzi (1972) and BSC, but not to GCRV.


457)   HIP  97278 = FK  741

   1 companion in CCDM+WDS:
B(1908: 133", 258 deg, 10.8 mag; pc).
Radial velocity is variable according to BSC.


458)   HIP  97290 = FK 1517

   Radial velocity is variable according to BSC.


459)   HIP  97421 = FK  739

   1 companion in TYCHO:
B(1991: 102", 333 deg,  9.49 mag; oo).
Radial velocity is variable according to W. Buscombe and P.M. Morris
(1961, Monthly Not. Roy. Astron. Soc.  123, 233).


460)   HIP  97804 = FK  746

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Note in HIP photometry: Appears double from a comparison between AC and DC
magnitudes. Cepheid. The pulsation explains the observed radial-velocity
variations. N.R. Evans (1992, Astrophys. J. 384, 220) lists a
'photometric companion'.


461)   HIP  97871 = FK 1519

   Radial velocity is variable according to BSC.


462)   HIP  98495 = FK  748

   Radial velocity may be variable according to BSC.


463)   HIP  98688 = FK  753

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC.


464)   HIP  99120 = FK  755

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


465)   HIP  99303 = FK 1525

   2 companions in TYCHO:
B(1991:  82", 122 deg,  9.37 mag; pc), C(1991: 104",  44 deg, 10.49; mag pc).
Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.
Barbier-Brossat (1989) gives v_rad = -7.9 km/s (Field 17: -13.6 km/s).


466)   HIP  99655 = FK  758

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


467)   HIP  99742 = FK 1526

   Radial velocity may be variable according to BSC.


468)   HIP  99951 = FK  760

   Radial velocity is variable according to BSC.


469)   HIP 100062 = FK 1529

   Radial velocity may be variable according to BSC.


470)   HIP 100151 = FK 1528

   Radial velocity may be variable (J. Andersen and B. Nordstroem, 1983, Astron.
Astrophys. Suppl. Ser. 52, 479).


471)   HIP 101067 = FK 1535

   1 companion in TYCHO:
B(1991: 119", 282 deg, 10.49 mag; pc).


472)   HIP 101076 = FK 1534

   Radial velocity may be variable according to BSC.


473)   HIP 101101 = FK 1533

   Radial velocity is variable according to BSC.


474)   HIP 101134 = FK 1538

   Radial velocity may be variable according to BSC.


475)   HIP 101421 = FK  768

   Radial velocity is variable according to BSC.


476)   HIP 101489 = FK 1537

   Radial velocity is variable (J. Andersen and B. Nordstroem, 1983, Astron.
Astrophys. Suppl. Ser. 52, 479).


477)   HIP 101984 = FK  773

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


478)   HIP 102014 = FK 1540

   Radial velocity may be variable according to BSC.


479)   HIP 102098 = FK  777

   1 companion in CCDM+WDS:
B(1925:  75", 106 deg, 11.7 mag; pc).
Radial velocity is variable according to BSC.
HIP: percentage of rejected data F1 = 4%.


480)   HIP 102208 = FK  915

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


481)   HIP 102333 = FK  776

   The spectral type is variable (S. Malaroda, 1973, Publ. Astron. Soc. Pacific
85, 328), but no indications of radial-velocity variations.


482)   HIP 102485 = FK  779

   Radial velocity is variable according to BSC.


483)   HIP 102618 = FK  781

   Radial velocity may be variable according to BSC.


484)   HIP 102624 = FK 1543

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


485)   HIP 102770 = FK 1545

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


486)   HIP 102978 = FK 1546

   Radial velocity is variable according to BSC.


487)   HIP 103200 = FK  786

   1 companion in TYCHO:
B(1991: 102",  81 deg,  9.83 mag; pc).
Radial velocity may be variable according to BSC.


488)   HIP 103460 = FK 1548

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


489)   HIP 103682 = FK  789

   Radial velocity may be variable according to BSC.


490)   HIP 103882 = FK  790

   1 companion in TYCHO:
B(1991: 100", 207 deg, 10.71 mag; oo).
Radial velocity may be variable according to BSC.


491)   HIP 104105 = FK  795

   Radial velocity is variable
according to GCRV, BSC, and Sinzi (1972). Barbier-Brossat (1989) gives
v_rad = -22.5 km/s (Field 17: -16 km/s).


492)   HIP 104139 = FK 1552

   BSC claims that the radial velocity is variable.
However, the orbital elements (H.A. Abt, 1961, Astrophys. J. Suppl. Ser.
6, 37) given in the remarks of BSC refer to Theta Cep (instead of
Theta Cap). Probably a misidentification in BSC and SIMBAD.


493)   HIP 104189 = FK 1553

   The radial velocity is variable according to J. Andersen and B. Nordstroem
(1983, Astron. Astrophys. Suppl. Ser. 52, 479).


494)   HIP 104755 = FK 1554

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


495)   HIP 105140 = FK  801

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1961, Monthly Not. Roy. Astron. Soc.  123, 233) and to W. Buscombe
(1963, Monthly Not. Roy. Astron. Soc.  126, 29).
Barbier-Brossat (1989) gives v_rad = +7.2 km/s (Field 17: -1 km/s).


496)   HIP 105199 = FK  803

   3 companions in CCDM+WDS:
B(1908: 207",  22 deg, 10.4 mag; af), C(B(CD): 1908: 20", 172 deg, 11.1 mag; oo),
D(CD: 1908:   3", 104 deg, 11.3 mag).
Radial velocity is variable according to BSC.


497)   HIP 105515 = FK 1561

   According to HIP: eclipsing binary (type:EA) with a possible period of 4.1221
days. HIP does not confirm the period of 68.0 days obtained by G.L. Henry et
al. (1995, Astron. J.  110, 2926) from their photometry. The radial
velocity is constant according to G.L. Henry et al., who interpret the period
of 68 days as the rotational period of the star indicated by stellar spots.


498)   HIP 105858 = FK  805

   Radial velocity is variable
according to Sinzi (1972), but K.A. Murdoch et al. (1993, Astrophys. J. 413,
349) do not find any significant variations in the radial velocity.


499)   HIP 106021 = FK 1564

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


500)   HIP 106093 = FK  807

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.


501)   HIP 106429 = FK 1567

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


502)   HIP 106787 = FK 1570

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.
Barbier-Brossat (1989) gives v_rad = -35.8 km/s (Field 17: -25 km/s).


503)   HIP 107315 = FK  815

   2 companions in CCDM+WDS:
B(1961:  83", 324 deg, 12.7 mag; af), C(1914: 143", 321 deg,  8.9 mag; pc).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC.


504)   HIP 107418 = FK 1572

   Radial velocity is variable according to BSC.


505)   HIP 107445 = FK 1571

   1 companion in TYCHO:
B(1991:  93",  22 deg,  10.70 mag; oo).


506)   HIP 107517 = FK  818

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


507)   HIP 107575 = FK 1574

   Radial velocity may be variable according to BSC.


508)   HIP 107649 = FK 1573

   1 companion in CCDM+WDS:
B(1932:  55", 356 deg,  8.6 mag; nc).
Tycho gives for B (1991:  73", 351 deg,  8.65 mag).


509)   HIP 108022 = FK  823

   Radial velocity may be variable according to E.B. Frost et al. (1926,
Astrophys. J. 64, 1) and to H.A. Abt et al. (1990, Astrophys. J. 74, 551).
K. Kodaira (1971, Publ. Astron. Soc. Japan  23, 159)
determined a period of 17.79 days, but remarked
that the scatter in many of the data is extraordinarily
large. Duplicity uncertain. v_rot sin(i) ~150 km/s.


510)   HIP 108036 = FK 1577

   Radial velocity is variable according to BSC.
HIP: percentage of rejected data F1 = 4%.


511)   HIP 109074 = FK  827

   1 companion in CCDM+WDS:
B(1907: 113",  41 deg, 12.2 mag; pc).
Radial velocity may be variable according to BSC.
and to T.G. Barnes et al. (1986, Publ. Astron. Soc. Pacific  98, 223).


512)   HIP 109139 = FK  828

   Double-lined spectroscopic binary (e.g.: E.B. Frost et al., 1926, Astrophys. J.
64, 1; W.W. Campbell and J.H. Moore, 1928, Publ. Lick Obs.  16, 321).


513)   HIP 109400 = FK  837

   Radial velocity is variable according to BSC.


514)   HIP 109492 = FK  836

   Suspected spectroscopic binary (e.g.: J. Moore, 1932, Publ. Lick Obs.  18,
especially p. 212; K.C. Gordon, 1943, Publ. Astron. Soc. Pacific  55,
100; G. Burki and M. Mayor, 1983, Astron. Astrophys. 124, 256).


515)   HIP 110256 = FK  839

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


516)   HIP 110386 = FK  843

   Radial velocity may be variable according to BSC.
Barbier-Brossat (1989) gives v_rad = +1 km/s (Field 17: +9.6 km/s).


517)   HIP 110672 = FK 1585

   Radial velocity is variable according to BSC.


518)   HIP 110986 = FK 1588

   Radial velocity may be variable according to BSC.


519)   HIP 110992 = FK 1589

   Radial velocity is variable according to BSC.


520)   HIP 111056 = FK 1593

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).


521)   HIP 111196 = FK 1670

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609).


522)   HIP 111242 = FK 1594

   Radial velocity is variable (e.g.: R. Woolley et al., 1981,
Royal Obs. Ann. No. 14, p. 5).


523)   HIP 111497 = FK  850

   Radial velocity is variable according to Sinzi (1972)
or may be variable according to BSC, but not to GCRV.


524)   HIP 111532 = FK  851

   Radial velocity is variable according to BSC.


525)   HIP 111710 = FK 1595

   1 companion in CCDM+WDS:
B(1926:  98", 248 deg,  8.8 mag; nc).
Tycho gives for B (1991:  87", 250 deg, 11.14 mag).


526)   HIP 111797 = FK  853

   Radial velocity is variable according to GCRV, BSC, and Sinzi (1972).
BSC gives SB2.


527)   HIP 111841 = FK  852

   1 companion in CCDM+WDS:
B(1975:  62",  49 deg, 10.0 mag; pc).
TYCHO gives for B(1991:  62",  49 deg, 10.29 mag).
Radial velocity may be variable according to BSC.


528)   HIP 112029 = FK  855

   2 companions in CCDM+WDS:
B(1925:  62", 140 deg, 11.6 mag; nc), C(1880: 177",   5 deg, 11. mag; oo).
Radial velocity may be variable according to BSC.


529)   HIP 112122 = FK  856

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).


530)   HIP 112358 = FK 1596

   Radial velocity may be variable according to BSC.


531)   HIP 112623 = FK  860

   1 companion in TYCHO:
B(1991:  96",  68 deg, 10.52 mag; oo).
Radial velocity is variable according to W. Buscombe and P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609).


532)   HIP 112716 = FK  861

   1 companion in CCDM+WDS:
B(1963: 132", 296 deg,  9.8 mag; af).


533)   HIP 113881 = FK  870

   2 companions in CCDM+WDS:
B(1925: 109", 211 deg, 11.8 mag; af), C(1925: 253",  98 deg,  9.6 mag; af).
Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity is variable according to BSC.


534)   HIP 113963 = FK  871

   Radial velocity is variable according to BSC.


535)   HIP 114210 = FK 1604

   Radial velocity may be variable according to BSC.


536)   HIP 114520 = FK 1606

   Radial velocity is variable according to BSC.


537)   HIP 114622 = FK  875

   1 companion in CCDM+WDS:
B(1922: 124", 218 deg,  9.4 mag; af).
Radial velocity is constant according to G.A.H. Walker et al.
(1995, Icarus  116, 359).


538)   HIP 114971 = FK  878

   Radial velocity may be variable according to BSC.


539)   HIP 115250 = FK  880

   Radial velocity is variable according to BSC.
Delta Scuti star. The pulsation explains the observed radial-velocity variations.


540)   HIP 115280 = FK 1610

   2 companions in CCDM+WDS:
B(1922: 122", 256 deg,  9.2 mag; af), C(BC: 1908: 156", 214 deg, 11.5 mag; oo).
Radial velocity may be variable according to BSC.


541)   HIP 115438 = FK 1612

   Radial velocity is variable according to BSC.


542)   HIP 115590 = FK  882

   3 companions in CCDM+WDS:
B(1918:  98", 225 deg,  7.8 mag; nc, pc), C(1918: 215", 258 deg,  8.7 mag; pc),
D(CD: 1913:   9",  34 deg,  9.7 mag).
TYCHO gives for B(1991:  96", 226 deg, 9.82 mag).


543)   HIP 115591 = FK 1613

   Radial velocity is variable according to BSC.


544)   HIP 115713 = FK  883

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1961, Monthly Not. Roy.
Astron. Soc.  123, 233).


545)   HIP 115738 = FK  884

   2 companions in CCDM+WDS:
B(1950: 163", 344 deg, 11.9 mag; nc), C(BC: 1908:  76", 154 deg, 13.1 mag; oo).
Radial velocity and spectrum are variable (e.g.: P. Galeotti and E. Lovera,
1972, Mem. Soc. Astron. Italiana  43, 759).


546)   HIP 116354 = FK 1616

   Radial velocity is variable according to BSC.


547)   HIP 116602 = FK  889

   Radial velocity is variable
according to W. Buscombe and P.M. Morris (1958, Monthly Not. Roy.
Astron. Soc.  118, 609) and to W. Buscombe (1963, Monthly Not. Roy.
Astron. Soc.  126, 29). Barbier-Brossat (1989) gives
v_rad = +3.4 km/s (Field 17: +10 km/s).


548)   HIP 116631 = FK  891

   In spite of other claims (e.g. BSC),
the radial velocity is probably constant (e.g. GCRV).
v_rot  sin(i) ~90 km/s.


549)   HIP 116771 = FK  892

   2 companions in CCDM+WDS:
B(1910:  70", 295 deg, 13.0 mag; af), C(1880: 281",  34 deg; oo).
Radial velocity may be variable according to T.G. Barnes et al. (1986,
Publ. Astron. Soc. Pacific  98, 223).


550)   HIP 116820 = FK 1618

   1 companion in TYCHO:
B(1991:  97",  34 deg, 10.98 mag; oo).


551)   HIP 116928 = FK 1620

   Radial velocity is variable according to BSC.


552)   HIP 117089 = FK 1621

   Radial velocity is variable according to W. Buscombe and P.M. Morris
(1958, Monthly Not. Roy. Astron. Soc.  118, 609) and to D. Baade
(1989, Astron. Astrophys. Suppl. Ser. 79, 423). v_rot sin(i) ~315 km/s.


553)   HIP 117371 = FK  895

   Radial velocity is variable according to BSC.


554)   HIP 117375 = FK 1623

   2 companions in CCDM+WDS:
B(1919: 173", 285 deg, 10.0 mag; nc:), C(BC: 1912:  52", 278 deg, 12.9 mag; AC: pc).
Radial velocity may be variable according to BSC.


555)   HIP 117488 = FK 1624

   Radial velocity may be variable (J. Andersen and B. Nordstroem, 1983, Astron.
Astrophys. Suppl. Ser. 52, 479).


556)   HIP 117541 = FK  897

   Radial velocity is variable according to BSC.


557)   HIP 117718 = FK  898

   Suspected by HIP to be double or multiple (Flag S in HIP Field H61).
Radial velocity may be variable according to BSC.


558)   HIP 117863 = FK  899

   1 companion in TYCHO:
B(1991:  93", 149 deg, 10.62 mag; pc).
Radial velocity is variable according to BSC.
G. Burki and M. Mayor (1983, Astron. Astrophys. 124, 256) classified
the star as a possible spectroscopic binary.
The spectrum is variable. Double lines in the spectrum of rho Cas
are probably not due to binarity but caused by effects in the stellar
atmosphere (W.P. Bidelman and A. McKellar, 1957, Publ. Astron. Soc. Pacific
69, 31; D.L. Lambert et al., 1981, Astrophys. J. 248, 638).


559)   HIP 118048 = FK 1628

   1 companion in TYCHO:
B(1991:  62",  0 deg, 10.13 mag; oo).
Radial velocity may be variable according to BSC.


560)   HIP 118268 = FK  902

   The object was announced as a spectroscopic binary by H. Spencer-Jones (1928,
Ann. Cape. Obs. 10, Part 8, p. 129). A preliminary orbital period of 2.158 days
was given by W.R. Beardsley (1965, Astron. J. 70, 318). This was not confirmed
by H.A. Abt and S.G. Levy (1976, Astrophys. J. Suppl. Ser. 30, 273).
W.B. Lee et al. (1985, Astron. Astrophys. Suppl. Ser. 61, 363) found also no
periodicity in the radial velocity and think that the variations, if existing,
are not due to duplicity.


3001)    HIP   7007     FK 2099

The radial velocity is probably constant. The star is used as a radial-velocity
standard by many authors.


3002)    HIP  12048     FK 4237

The star has a planetary companion according to G.W. Marcy et al. (2000,
Astrophys. J. 536, L43).


3003)    HIP  19554     FK 2301

Radial velocity is variable according to R.F. Griffin et al. (1988, Astron. J.
96, 172).


3004)    HIP  20715     FK 2327

S. Wolff (1978, Astrophys. J. 222, 556) considered the star to be a
spectroscopic binary with an orbital period of 2.48 or 4.95 days. The star is
a slowly pulsating B star with a photometric period of 1.08 days
(C. Waelkens et al., 1998, Astron. Astrophys. 330, 215).


3005)    HIP  25041     FK 2401

Spectroscopic binary with an orbital period of 4.1707 days. No other orbital
elements are given by N. Morrell and H. Levato (1991, Astrophys. J. Suppl. Ser.
75, 965).


3006)    HIP  25302     FK 2406

Radial velocity is variable according to N. Morrell and H. Levato (1991,
Astrophys. J. Suppl. Ser. 75, 965).

3007)    HIP  26093     FK 2414

Radial velocity is constant according to H.A. Abt et al. (1990, Astrophys. J.
Suppl. Ser. 74, 551).


3008)    HIP  26248     FK 2415

Radial velocity is constant according to H.A. Abt et al. (1990, Astrophys. J.
Suppl. Ser.  74, 551).


3009)    HIP  26594     FK 2423

Radial velocity is variable according to N. Morrell and H. Levato (1991,
Astrophys. J. Suppl. Ser. 75, 965).


3010)    HIP  32864     FK 2523

Radial velocity is constant according to H.A. Abt et al. (1990, Astrophys. J.
Suppl. Ser. 74, 551).


3011)    HIP  34495     FK 2551

The SIMBAD classification of this star as a Cepheid seems to be unjustified.


3012)    HIP  60500     FK 5094

The star was claimed to be a close visual binary with a separation of less than
0.3" by Maedler (Omicron-Sigma 248). Other observers did not confirm this
binarity (W.J. Hussey, 1901, Publ. Lick Obs. 5, 113). However, HIPPARCOS
also suspects the star to be double (Flag S in HIP Field H61).


3013)    HIP  62027     FK 3015

X-ray binary according to C. Chevalier and S.A. Ilovaisky (1998, Astron.
Astrophys. 330, 201).


3014)    HIP  64408     FK 3051

Radial velocity is constant according to K.A. Murdoch et al. (1993, Astrophys.
J. 413, 349).


3015)    HIP  70218     FK 5267

Radial velocity may be variable with a long period according to A. Young et al.
(1987, Astrophys. J. 314, 272).


3016)    HIP  72339     FK 5310

The star has a planetary companion according to S. Udry et al. (2000, Astron.
Astrophys. 356, 590).


3017)    HIP  91499     FK 3485

Radial velocity may be variable according to G. Burki and M. Mayor (1983,
Astron. Astrophys. 124, 256) and A.M. Valitova et al. (1990, Sov. Astron.
Lett. 16, 301).


3018)    HIP  93015     FK 3505

kappa Pav is a Cepheid of the W Virginis type. In addition to its pulsation,
the star is probably a spectroscopic binary according to G. Wallerstein et al.
(1992, Monthly Not. Roy. Astron. Soc. 259, 474).


3019)    HIP  94083     FK 3536

Radial velocity may be variable according to A. Duquennoy and M. Mayor (1991,
Astron. Astrophys. 248, 485).


3020)    HIP  96183     FK 5721

Radial velocity may be variable according to A. Duquennoy and M. Mayor (1991,
Astron. Astrophys. 248, 485).


3021)    HIP 104185     FK 3687

Cepheid DT Cyg. The star has a photometric companion according to L. Szabados
(1991, Commun. Konkoly Obs. No. 96).


3022)    HIP 105665     FK 3707

Radial velocity is probably constant. The star is used as a radial-velocity
standard by many authors.


3023)    HIP 110882     FK 3796

Radial velocity is probably constant. The star is used as a radial-velocity
standard by many authors.


3024)    HIP 113561     FK 3839

The star has a photometric companion seen in the ultraviolet according to S.B.
Parsons (1983, Astrophys. J. Suppl. Ser. 53, 553).



Updated: 23 April 2002