The range of core size of postcollapse clusters supported by primordial binaries
- 1 August 1994
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 431 (1) , 231-236
- https://doi.org/10.1086/174480
Abstract
We investigate how the core size of globular clusters in a postcollapse phase driven by primordial binaries depends upon the parameters of the distribution of the binary binding energy and the abundance of the binaries. We show that the variation of these quantities increases the plausible range for the core size.Keywords
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