The slowest spinning X-ray pulsar in an extragalactic globular cluster
The slowest spinning X-ray pulsar in an extragalactic globular cluster
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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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Contents
Neutron stars are thought to be born rapidly rotating and then exhibit a phase of a rotation-powered pulsations as they slow down to 1-10 s periods. The significant population of millisecond pulsars observed in our Galaxy is explained by the recycling concept: during an epoch of accretion from a donor star in a binary system, the neutron star is sp...
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Full title
The slowest spinning X-ray pulsar in an extragalactic globular cluster
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TN_cdi_proquest_journals_2075372340
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2075372340
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1602.05191
