Probing clumpy stellar winds with a neutron star
INTEGRAL tripled the number of super-giant high-mass X-ray binaries (sgHMXB) known in the Galaxy by revealing absorbed and fast transient (SFXT) systems. Quantitative constraints on the wind clumping of massive stars can be obtained from the study of the hard X-ray variability of SFXT. A large fract...
Main Authors: | , , |
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Format: | Others |
Language: | English |
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Universität Potsdam
2007
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Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18024 http://opus.kobv.de/ubp/volltexte/2008/1802/ |