The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies 1988
DOI: 10.1007/978-94-015-1104-9_40
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“…How long it takes for the binary to turn into an X-ray source then depends on the time required for the orbit to shrink due to loss of angular momentum, or for the donor to expand into a giant after completing its main-sequence evolution (for reviews see and Chapter 16 by Tauris and Van den Heuvel). It may be noted that binaries formed in a globular cluster may also go through a long-lived detached phase (Grindlay 1988). …”
Section: Comparison Between Field and Cluster Sourcesmentioning
confidence: 99%
“…How long it takes for the binary to turn into an X-ray source then depends on the time required for the orbit to shrink due to loss of angular momentum, or for the donor to expand into a giant after completing its main-sequence evolution (for reviews see and Chapter 16 by Tauris and Van den Heuvel). It may be noted that binaries formed in a globular cluster may also go through a long-lived detached phase (Grindlay 1988). …”
Section: Comparison Between Field and Cluster Sourcesmentioning
confidence: 99%