The Initial Stellar Mass Function as a Statistical Ensemble and Implications for the Formation of Bound Clusters

Details The Initial Stellar Mass Function as a Statistical Ensemble and Implications for the Formation of Bound Clusters The Initial Stellar Mass Function as a Statistical Ensemble and Implications for the Formation of Bound Clusters

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..235e&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Physics

2

Scientific paper

Statistical aspects of the inital stellar mass function and star formation in clusters are considered. The basic physical properties of galactic clusters may result from a random selection of stellar masses during the star formation process in a cloud core, combined with an epoch of cloud disruption at the time of formation of a sufficiently massive star.

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