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تسجيل مستخدم جديدDense Stellar Populations: Initial Conditions
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Pavel Kroupa
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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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