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The Dark Side of Globular Clusters
Published online by Cambridge University Press: 25 May 2016
Abstract
Searches of low-mass stars have become possible in globular clusters, and the first results suggest that the mass function turns up below ∼ 0.4 M⊙ (Fahlman et al. 1989; Richer et al., 1990; Richer et al. 1991; G. Piotto, these proceedings). This conclusion is independently supported by the non-parametric dynamical analysis of four clusters by Gebhardt and Fisher 1995.
- Type
- Stellar Dynamics, Models
- Information
- Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 377 - 378
- Copyright
- Copyright © Kluwer 1996