Optically thick envelopes around ULXs powered by accreating neutron stars
Optically thick envelopes around ULXs powered by accreating neutron stars
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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
Magnetized neutron stars power at least some ultra-luminous X-ray sources. The accretion flow in these cases is interrupted at the magnetospheric radius and then reaches the surface of a neutron star following magnetic field lines. Accreting matter moving along magnetic field lines forms the accretion envelope around the central object. We show tha...
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Full title
Optically thick envelopes around ULXs powered by accreating neutron stars
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TN_cdi_proquest_journals_2074768040
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074768040
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1612.00964
