arXiv · 1501.02777
Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT
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.
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M. Orlandini, V. Doroshenko, L. Zampieri, E. Bozzo, A. Baykal, P. Blay, M. Chernyakova, R. Corbet, A. D'Aì, T. Enoto, C. Ferrigno, M. Finger, D. Klochkov, I. Kreykenbohm, S. C. Inam, P. Jenke, J. -C. Leyder, N. Masetti, A. Manousakis, T. Mihara, B. Paul, K. Postnov, P. Reig, P. Romano, A. Santangelo, N. Shakura, R. Staubert, J. M. Torrejón, R. Walter, J. Wilms, C. Wilson-Hodge. 2015-01-12. Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT. https://arxiv.org/abs/1501.02777
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