Population of dynamically formed triples in dense stellar systems

Details Population of dynamically formed triples in dense stellar systems Population of dynamically formed triples in dense stellar systems

2005-09-18

arxiv.org/abs/astro-ph/0509516v1

Astronomy and Astrophysics

Astrophysics

6 pages, 5 figures, ESO Workshop "Multiple Stars across the H-R Diagram", held in Garching, Germany, 12-15 July 2005

Scientific paper

In dense stellar systems, frequent dynamical interactions between binaries lead to the formation of multiple systems. In this contribution we discuss the dynamical formation of hierarchically stable triples: the formation rate, main characteristics of dynamically formed population of triples and the impact of the triples formation on the population of close binaries. In particular, we estimate how much the population of blue stragglers and compact binaries could be affected.

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