The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities
published by Lorenzo Ducci
in 2010
in Physics
and research's language is
English
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Abstract in English
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).