A study of the accretion mechanisms of the High Mass X-ray Binary IGR J00370+6122
A study of the accretion mechanisms of the High Mass X-ray Binary IGR J00370+6122
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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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Contents
IGR J00370+6122 is a high-mass X-ray binary, of which the primary is a B1 Ib star, whereas the companion is suggested to be a neutron star by the detection of 346-s pulsation in one-off 4-ks observation. To better understand the nature of the compact companion, the present work performs timing and spectral studies of the X-ray data of this object,...
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A study of the accretion mechanisms of the High Mass X-ray Binary IGR J00370+6122
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TN_cdi_proquest_journals_2556169046
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2556169046
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2107.12633
