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arXiv · 0801.3863

Supergiant Fast X-ray Transients and Other Wind Accretors

Ignacio Negueruela·Jose Miguel Torrejon·Pablo Reig·Marc Ribo·David M. Smith
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Abstract

Supergiant Fast X-ray Transients are obviously related to persistent Supergiant X-ray Binaries. Any convincing explanation for their behaviour must consistently take into account all types of X-ray sources powered by wind accretion. Here we present a common framework for wind accreting sources, within the context of clumpy wind models, that allows a coherent interpretation of their different behaviours as an immediate consequence of diverse orbital geometries.

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Ignacio Negueruela, Jose Miguel Torrejon, Pablo Reig, Marc Ribo, David M. Smith. 2008-01-25. Supergiant Fast X-ray Transients and Other Wind Accretors. https://doi.org/10.1063/1.2945052

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