On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars
On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars
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Full title
Author / Creator
Takata, J , Cheng, K S and Taam, R E
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
The heating associated with the deposition of \(\gamma\)-rays in an accretion disk is proposed as a mechanism to facilitate the transformation of a low mass X-ray binary to the radio millisecond pulsar phase. The \(\gamma\)-ray emission produced in the outer gap accelerator in the pulsar magnetosphere likely irradiates the surrounding disk, resulti...
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Full title
On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars
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Record Identifier
TN_cdi_proquest_journals_2082539129
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082539129
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1009.4781