Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
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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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It has been recently discovered that the transition of X-ray pulsars to the low luminosity state (\(L\lesssim10^{35}\,{\rm erg\,s^{-1}}\)) is accompanied by a dramatic spectral change. Namely, the typical power-law-like spectrum with high energy cutoff transforms into a two-component structure with a possible cyclotron absorption feature on top of...
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Full title
Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte-Carlo approach
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TN_cdi_proquest_journals_2417175672
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2417175672
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2006.13596
