Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT
Date Issued
2015
Author(s)
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Doroshenko, V.
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Bozzo, E.
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Baykal, A.
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Blay, P.
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Chernyakova, M.
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Corbet, R.
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Enoto, T.
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Ferrigno, C.
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Finger, M.
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Klochkov, D.
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Kreykenbohm, I.
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Inam, S. C.
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Jenke, P.
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Leyder, J. -C.
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Manousakis, A.
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Mihara, T.
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Paul, B.
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Postnov, K.
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Reig, P.
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Santangelo, A.
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Shakura, N.
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Staubert, R.
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Torrejón, J. M.
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Walter, R.
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Wilms, J.
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Wilson-Hodge, C.
Abstract
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.
Rights
open.access
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