Formation of Ultracompact X-ray Binaries in Dense Star Clusters
Formation of Ultracompact X-ray Binaries in Dense Star Clusters
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Author / Creator
Ivanova, N , Rasio, F A , Lombardi, J C , Jr , Dooley, K L and Proulx, Z F
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
Bright, ultracompact X-ray binaries observed in dense star clusters, such as Galactic globular clusters, must have formed relatively recently, since their lifetimes as persistent bright sources are short (e.g., ~10^8 yr above 10^36 erg/s for a 1.4 Msun neutron star accreting from a degenerate helium companion with an initial mass of ~0.2 Msun). The...
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Full title
Formation of Ultracompact X-ray Binaries in Dense Star Clusters
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Record Identifier
TN_cdi_proquest_journals_2086279412
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2086279412
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E-ISSN
2331-8422
DOI
10.48550/arxiv.0501617