Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744-28 using t...
Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis
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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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The X-ray pulsar GRO J1744-28 is a unique source which shows both pulsations and type-II X-ray bursts, allowing studies of the interaction of the accretion disk with the magnetosphere at huge mass accretion rates exceeding \(10^{19}\) g s\(^{-1}\) during its super-Eddington outbursts. The magnetic field strength in the source, \(B\approx 5\times 10...
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Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis
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TN_cdi_proquest_journals_2225508893
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2225508893
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1905.05593
