Astronomisches Rechen-Institut Heidelberg

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Paper 2001028

Author(s): Khalisi, E.
Title: Shortening of core collapse time in star clusters with two masses
Source: In: European astronomy at the turn of the millennium. Proc. Joint European and Natl. Astron. Meeting (JENAM-2000), Moscow, 29 May - 3 June 2000; to appear in: Astron. Astrophys. Trans. [Abstr. in: JENAM-2000 Abstr. Book; ISBN 5-89118-124-X, GEOS, Moscow (2000), 54]
Year: 2001
Abstract: We present high accuracy N-body simulations of isolated star clusters consisting of two distinct mass components, m1 and m2 and vary their relative ratio μ = m2/m1. The mass fraction of the more massive component relative to the total mass, q = M2/Mtot, is set equal to 0.1 in all cases. We determine the average star mass within a fixed "Lagrangian shell". It is found that the time of first core collapse is reduced by the ratio μ with respect to a cluster with uniform masses.
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