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SXP 15.6 -- an accreting pulsar close to spin equilibrium?

SXP 15.6 -- an accreting pulsar close to spin equilibrium?

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2656453401

SXP 15.6 -- an accreting pulsar close to spin equilibrium?

About this item

Full title

SXP 15.6 -- an accreting pulsar close to spin equilibrium?

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2022-04

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

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,...

Alternative Titles

Full title

SXP 15.6 -- an accreting pulsar close to spin equilibrium?

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2656453401

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2656453401

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2204.12960

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