Dynamics of multiple stars

Details Dynamics of multiple stars Dynamics of multiple stars

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..75...17r&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 75, p. 17 - 25 (2003). In: Proceedings of the XII

Physics

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Physics Of Stars, Stellar Systems, Multiple Stars: Dynamics

Scientific paper

According to modern views, a majority of stars in galactic disk were formed within the small stellar groups containing a few components. As a rule, such groups have a non-hierarchical structure and decay. As a result, single, binary and stable multiple systems are formed. Binaries and stable triples - products of small group dynamical decay - have rather wide intervals of orbital parameters and mass ratios. This is in agreement with observations of double and multiple stars. We study the effects of star merging, dynamical friction on interstellar medium, and mass-loss to dynamical evolution of small stellar groups.

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