arXiv · astro-ph/0509516
Population of dynamically formed triples in dense stellar systems
Abstract
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Natalia Ivanova. 2005-09-18. Population of dynamically formed triples in dense stellar systems. https://arxiv.org/abs/astro-ph/0509516
Cite the original work for its findings. Save a collection to share your selection of sources.