SXP 15.6 -- an accreting pulsar close to spin equilibrium?
SXP 15.6 -- an accreting pulsar close to spin equilibrium?
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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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SXP 15.6 is a recently established Be star X-ray binary system (BeXRB) in the Small Magellanic Cloud (SMC). Like many such systems the variable X-ray emission is driven by the underlying behaviour of the mass donor Be star. It is shown here that the neutron star in this system is exceptionally close to spin equilibrium averaged over several years,...
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SXP 15.6 -- an accreting pulsar close to spin equilibrium?
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TN_cdi_proquest_journals_2656453401
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2656453401
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2204.12960