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First results from the use of the relativistic and slim disc model SLIMULX in XSPEC
DOI: 10.48550/arXiv.1705.07859 Bibcode: 2017CoSka..47...84C

Castro-Tirado, A. J.; Dovčiak, M.; Karas, V. +3 more

Ultra-Luminous X-ray sources (ULXs) are accreting black holes for which their X-ray properties have been seen to be different to the case of stellar-mass black hole binaries. For most of the cases their intrinsic energy spectra are well described by a cold accretion disc (thermal) plus a curved high-energy emission components. The mass of the blac…

2017 Contributions of the Astronomical Observatory Skalnate Pleso
XMM-Newton 4