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Dynamical Masses and Mass-to-Light Ratios for Globular Clusters

Published online by Cambridge University Press:  14 August 2015

G. Illingworth
G. Illingworth*
Affiliation:
Kitt Peak National Observatory, Tucson, Arizona, U.S.A.∗

Abstract

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Dynamical masses have been determined for 10 globular clusters. Comparison of the dynamically determined M/L values with those calculated from extrapolations of the observed upper main sequence/giant branch luminosity functions for M3 and M5 indicate that low mass stars (∼0.2 M⊙) comprise a large fraction of the total number.

Type
Part I/Spherical Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 151 - 157
Copyright
Copyright © Reidel 1975 

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