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On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars

On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082539129

On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars

About this item

Full title

On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars

Author / Creator

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2010-09

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

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...

Alternative Titles

Full title

On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars

Authors, Artists and Contributors

Identifiers

Primary Identifiers

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

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