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arxiv 1501.02777 v2 pith:RRVVMN3I submitted 2015-01-12 astro-ph.HE

Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT

classification astro-ph.HE
keywords x-rayloftbinarieshigh-massmissionsourcesultra-luminousaccretion
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This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of high-mass X-ray binaries and ultra-luminous X-ray sources. For a summary, we refer to the paper.

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