FK6 Part III

Explanation of tabular notes


Field FK:
FK number (See the description of Field 1 of the FK6(III).)

Field HIP:
HIPPARCOS number (See the description of Field 2 of the FK6(III).)

Field Tabular Note:

Columns H to V:
Indicators for binarity

Column H:
HIPPARCOS indicators for a suspected visual binary:
        s = Flag S in HIP Field H61.
        d = Flag D in HIP Field H52, based on photometry. This
            could be an indication of duplicity.
        t = HIP Flags S and D (t = s+d).

Column U:
HIPPARCOS percentage of rejected data (HIP Field H29, F1):
        percentage of rejected HIP data
        one digit: 0, 1, 2, ... percent)
A high percentage of rejected data may be caused by a duplicity of the object,
but other reasons cannot be excluded.

Column F:
HIPPARCOS goodness-of-fit parameter (HIP Field H30, F2):
        -        F2 < 0
        0   0 <= F2 < 1
        1   1 <= F2 < 2
        2   2 <= F2 < 3
        3   3 <= F2 < 4
        etc.
A large value of F2 (e.g. larger than 3) may be caused by a duplicity of
the object, but other reasons cannot be excluded.

Column K:
Indications on binarity provided by the catalogue of speckle observations
(Hartkopf et al. 1999).
        b = binary resolved by speckle (or other interferometric) observations
            (such objects are generally excluded from the FK6(III))
        u = possibly resolved
        n = object observed, but not resolved (i.e. no hint to binarity)

Column C:
Indicator for a star which has one (or more) visual component(s) with a
separation rho of at least 60".
Source of information:
        c = CCDM (Dommanget and Nys 1994)
        t = TYCHO2 (Hoeg et al. 2000)
        w = WDS (Worley and Douglass 1997, and updated versions under the given URL)
        r = other sources
Visual binaries with rho < 60" are generally excluded from the FK6(III).

Column G:
Indications on binarity provided by the General Catalogue of Stellar Radial
Velocities (GCRV, Wilson 1953):
        v = radial velocity is variable
        u = radial velocity may be variable
        2 = variable radial velocities for two stellar components
        b = (other) indications of binarity
        d = (other) indications of binarity are doubtful

Column B:
Indications on binarity provided by the Bright Star Catalogue (BSC, Hoffleit
and Jaschek 1982).
The symbols v, u, 2, b, d have the same meaning as explained for Column G.

Column S:
Indications on binarity provided by the radial-velocity bibliography given in
the data block 'oRV' of SIMBAD (CDS Strasbourg).
The symbols v, u, 2, b, d have the same meaning as explained for Column G.

Column T:
Indications on binarity provided by the spectral-type bibliography given in the
data block 'MK' of SIMBAD (CDS Strasbourg).
        b = binary
        u = possibly a binary

Column A:
Indications on binarity provided by the Third Bibliographic Catalogue of
Stellar Radial Velocities (Barbier-Brossat et al. 1994).
The symbols v, u, 2, b, d have the same meaning as explained for Column G.

Column M:
Indications on binarity provided by the Fourth Bibliographic Catalogue of
Stellar Radial Velocities (Malaroda et al. 2000).
The symbols v, u, 2, b, d have the same meaning as explained for Column G.
f = probably erroneous indication on binarity.

Column L:
Indications on binarity from additional literature (e.g. from papers more
recent than those used for Column M).
The symbols v, u, 2, b, d have the same meaning as explained for Column G.
c = radial velocity is probably constant.

Column V:
Indications on binarity from photometric variability.
        a = eclipsing binary, Algol type
        b = eclipsing binary, beta Lyrae type
        e = eclipsing binary, type uncertain
        w = eclipsing binary, W Ursae Majoris type

Column P:
Indicator for a variability of the radial velocity V_rad due to
stellar pulsation (which may be confused with a variability of
V_rad due to spectroscopic binarity).
        c = Cepheid
        s = delta Scuti star
        b = beta Cephei star

Column I:
        i = an individual note on this star is given in the
            'Individual Notes' of the FK6(III)

Field Indiv. Note:
Number of the individual note



Updated: 30 October 2000