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The influence of mass-loss from a star cluster on its dynamical friction – I. Clusters without internal evolution
Authors:M. Fellhauer   D. N. C. Lin
Affiliation:Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA;UCO/Lick Observatory, UC Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA
Abstract:
Keywords:methods: N-body simulations    galaxies: dwarf    galaxies: kinematics and dynamics    galaxies: star clusters
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