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

2); (2) INAF/IASF Milano (3) INAF/IASF Palermo; A. Paizis (2); Como; Italy); L. Ducci (1; L. Sidoli (2); P. Romano (3); S. Mereghetti (2) ((1) Universit\`a degli Studi dell'Insubria

arxiv: 1003.5829 · v1 · submitted 2010-03-30 · 🌌 astro-ph.HE

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

L. Ducci (1 , 2) , L. Sidoli (2) , P. Romano (3) , A. Paizis (2) , S. Mereghetti (2) ((1) Universit\`a degli Studi dell'Insubria , Como , (2) INAF/IASF Milano (3) INAF/IASF Palermo

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keywords x-raybinarieshighmassmodelwindbehaviourclasses

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

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