Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and r...
Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination
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Ithaca: Cornell University Library, arXiv.org
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English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
Neutron stars (NSs) in low-mass X-ray binaries rotate at frequencies high enough to significantly deviate from sphericity (\(\nu_* \sim\) 200--600 Hz). We investigate the effects of rapid rotation on the observational appearance of a NS. We propose analytical formulae relating gravitational mass and equatorial radius of the rapidly rotating NS to t...
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Full title
Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination
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TN_cdi_proquest_journals_2405422849
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2405422849
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2005.09759
