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

2015-01-01
Maoura, Orlandini
Maoura, Orlandini
Dorosheknko, Vi
Baykal, Altan
Vi, Dorosheknko
Orlandini, Maoura
Orlandini, Maoura
Orlandini, Maoura
Maoura, Orlandini
Orlandini, Maoura
Maoura, Orlandini
Orlandini, Maoura
Maoura, Orlandini
Orlandini, Maoura
Vi, Dorosheknko
Vi, Dorosheknko
Dorosheknko, Vi
Dorosheknko, Vi
Dorosheknko, Vi
Dorosheknko, Vi
Dorosheknko, Vi
Dorosheknko, Vi
Maoura, Orlandini
Maoura, Orlandini
Maoura, Orlandini
Orlandini, Maoura
Maoura, Orlandini
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.
Citation Formats
O. Maoura et al., “Probing stellar winds and accretion physics in high mass X ray binaries and ultra luminous X ray sources with LOFT,” pp. 1–21, 2015, Accessed: 00, 2021. [Online]. Available: http://adsabs.harvard.edu/abs/2015arXiv150102777O.