Accretion from a clumpy massive-star wind in supergiant X-ray binaries
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DOI: 10.1093/mnras/stx3211
Abstract: Supergiant X-ray Binaries (SgXB) host a compact object, often a neutron star (NS), orbiting an evolved O/B star. Mass transfer proceeds through the intense line-driven wind of the stellar donor, a fraction of which is… read more here.
Keywords: wind; accretion; supergiant ray; ray binaries ... See more keywords