Mass Segregation Influence on Weighting Young Star Clusters

Details Mass Segregation Influence on Weighting Young Star Clusters Mass Segregation Influence on Weighting Young Star Clusters

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..605f&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

Due to mass segregation, virial mass estimates of young star clusters can easily be biased by a factor of 2 within the first 100 Myrs of evolution. A full set of parameter space has been explored (total mass, Initial Mass Function, density, mass extend, stellar evolution, etc.) using a gas-dynamical model coupled with the Cambridge stellar evolution tracks. Observational implications are discussed.

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