Clumpy wind studies and the non-detection of cyclotron line in OAO 1657-415
Clumpy wind studies and the non-detection of cyclotron line in OAO 1657-415
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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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Winds of massive stars are suspected to be inhomogeneous (or clumpy), which biases the measures of their mass loss rates. In High Mass X-ray Binaries (HMXBs), the compact object can be used as an orbiting X-ray point source to probe the wind and constrain its clumpiness. We perform spectro-timing analysis of the HMXB OAO 1657-415 with non-simultane...
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Clumpy wind studies and the non-detection of cyclotron line in OAO 1657-415
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TN_cdi_proquest_journals_2779259838
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2779259838
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2331-8422
DOI
10.48550/arxiv.2302.10939
