The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

Details The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities

2010-03-30

arxiv.org/abs/1003.5829v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

To appear in the proceedings of 'The Shocking Universe', held in Venice on September 14-18, 2009

Scientific paper

We have developed a clumpy stellar wind model for OB supergiants in order to
compare predictions of this model with the X-ray behaviour of both classes of
persistent and transient High Mass X-ray Binaries (HMXBs).

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