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LMXB and IMXB Evolution: I. The Binary Radio Pulsar PSR J1614-2230

Abstract:

We have computed an extensive grid of binary evolution tracks to represent low- and intermediate mass X-ray binaries (LMXBs and IMXBs). The grid includes 42,000 models which covers 60 initial donor masses over the range of 1-4 solar masses and, for each of these, 700 initial orbital periods over the range of 10-250 hours. These results can be applied to understanding LMXBs and IMXBs: those that evolve analogously to CVs; that form ultracompact binaries with orbital periods in the range of 6-5...

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Publication status:
Published

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Publisher copy:
10.1088/0004-637X/732/2/70

Authors


Rappaport, S More by this author
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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
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Journal:
ASTROPHYSICAL JOURNAL
Volume:
732
Issue:
2
Pages:
70-70
Publication date:
2011-05-10
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
URN:
uuid:ae09213f-1910-4014-848e-d4e9a2a17712
Source identifiers:
138988
Local pid:
pubs:138988
Keywords:

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