Timescale of twin-peak quasi-periodic oscillations and mass of accreting neutron stars
Timescale of twin-peak quasi-periodic oscillations and mass of accreting neutron stars
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Einstein's general relativity predicts that orbital motion of accreted gas approaching a neutron star (NS) in a NS low-mass X-ray binary (LMXB) system occurs on a time scale proportional to the NS mass. Radiation of the gas accounts for most of the observed LMXBs variability. In more than a dozen of sources twin-peak quasi-periodic oscillations (QP...
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Timescale of twin-peak quasi-periodic oscillations and mass of accreting neutron stars
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TN_cdi_proquest_journals_2256345209
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2256345209
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1907.05174
