Long-period Pulsars as Possible Outcomes of Supernova Fallback Accretion
Long-period Pulsars as Possible Outcomes of Supernova Fallback Accretion
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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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For about half a century the radio pulsar population was observed to spin in the ~0.002-12s range, with different pulsar classes having a spin-period evolution that differs substantially depending on their magnetic fields or past accretion history. The recent detection of several slowly rotating pulsars has re-opened the long-standing question of t...
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Long-period Pulsars as Possible Outcomes of Supernova Fallback Accretion
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TN_cdi_proquest_journals_2623497324
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2623497324
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2201.11704
