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arXiv · 1003.5829

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

L. Ducci·L. Sidoli·P. Romano·A. Paizis·S. Mereghetti
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Abstract

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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L. Ducci, L. Sidoli, P. Romano, A. Paizis, S. Mereghetti. 2010-03-30. The X-ray flaring emission from High Mass X-ray Binaries: the effects of wind inhomogeneities. https://arxiv.org/abs/1003.5829

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