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Masses of black holes in binary stellar systems
Uspekhi Fizicheskih Nauk, 1996Mass determination methods and their results for ten black holes in X-ray binary systems are summarised. A unified interpretation of the radial velocity and optical light curves allows one to reliably justify the close binary system model and to prove the correctness of determination of the optical star mass function fv(m).The orbit plane inclination i
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Stellar-Mass Black Hole Binaries as ULXs
AIP Conference Proceedings, 2005Ultraluminous X‐ray sources (ULXs) with Lx > 1039 ergs s−1 have been discovered in great numbers in external galaxies with ROSAT, Chandra, and XMM‐Newton. The central question regarding this important class of sources is whether they represent an extension in the luminosity function of binary X‐ray sources containing neutron stars and stellar‐mass ...
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Intermediate-mass black holes from stellar mergers in young star clusters
Monthly Notices of the Royal Astronomical Society, 2021Michela Mapelli +2 more
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Dynamics of Dwarf Galaxies Disfavor Stellar-Mass Black Holes as Dark Matter
Physical Review Letters, 2017Savvas Koushiappas, Abraham Loeb
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Accretion-induced variability links young stellar objects, white dwarfs, and black holes
Science Advances, 2015Simone Scaringi +2 more
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