McScatter: Three-Body Scattering with Stellar Evolution

Details McScatter: Three-Body Scattering with Stellar Evolution McScatter: Three-Body Scattering with Stellar Evolution

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ascl.soft01001h&link_type=abstract

Astrophysics Source Code Library, record ascl:1201.001

Astronomy and Astrophysics

Astrophysics

Scientific paper

McScatter illustrates a method of combining stellar dynamics with stellar evolution. The method is intended for elaborate applications, especially the dynamical evolution of rich star clusters. The dynamics is based on binary scattering in a multi-mass field of stars with uniform density and velocity dispersion, using the scattering cross section of Giersz (MNRAS, 2001, 324, 218-30).

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