Dense Stellar Populations: Initial Conditions

Details Dense Stellar Populations: Initial Conditions Dense Stellar Populations: Initial Conditions

2008-03-12

arxiv.org/abs/0803.1833v1

Astronomy and Astrophysics

Astrophysics

85 pages. To appear in The Cambridge N-body Lectures, Sverre Aarseth, Christopher Tout, Rosemary Mardling (eds), Lecture Notes

Scientific paper

10.1007/978-1-4020-8431-7_8

This chapter is based on four lectures given at the Cambridge N-body school
"Cambody". The material covered includes the IMF, the 6D structure of dense
clusters, residual gas expulsion and the initial binary population. It is aimed
at those needing to initialise stellar populations for a variety of purposes
(N-body experiments, stellar population synthesis).

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