Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT
Orlandini, M. · Doroshenko, V. · Zampieri, L. · Bozzo, E. · Baykal, A. · Blay, P. · Chernyakova, M. · Corbet, R. · D'Aì, A. · Enoto, T. · Ferrigno, C. · Finger, M. · Klochkov, D. · Kreykenbohm, I. · Inam, S. C. · Jenke, P. · Leyder, J. -C. · Masetti, N. · Manousakis, A. · Mihara, T. · Paul, B. · Postnov, K. · Reig, P. · Romano, P. · Santangelo, A. · Shakura, N. · Staubert, R. · Torrejón, J. M. · Walter, R. · Wilms, J. · Wilson-Hodge, C.
الأصل · EN
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.
الترجمة العربية
لا توجد ترجمة عربية لهذا البحث بعد. كن أوّل من يطلبها: تستغرق ثوانيَ معدودة، وتُحفظ النتيجة لكل قارئ قادم.