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2009MNRAS.399.1471E - Mon. Not. R. Astron. Soc., 399, 1471-1481 (2009/November-1)
Towards multiple-star population synthesis.
EGGLETON P.P.
Abstract (from CDS):
This numerical model may be useful for (i) comparison with the results of star and star cluster formation theory, (ii) population synthesis that does not ignore multiplicity above 2 and (iii) initial conditions for dynamical cluster simulations.
Abstract Copyright: Journal compilation © 2009 RAS, No claim to original US government works
Journal keyword(s): stars: general - stars: statistics
Simbad objects: 7
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