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Accretion and outflow in black-hole x-ray binaries
Black hole X-ray binaries (BHXBs) are stellar binary systems consisting of a black hole (BH) and a companion star. They are known to produce X-ray emission through the accretion of mass from the companion star onto the black hole via an accretion disc, as well as radio emission originating from thei...
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| Language: | English |
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Department of Astronomy
2015
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