Black Hole Mass Determination In The X Ray Binary 4u 1630 47 Scaling Of Spectral And Variability Characteristics

Black Hole Mass Determination In The X Ray Binary 4u 1630 47 Scaling Of Spectral And Variability Characteristics

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a stellar black hole or stellar mass black hole is a black hole formed by the gravitational collapse of a star they have masses ranging from about 5 to several tens of solar masses the process is observed as a hypernova explosion or as a gamma ray burst these black holes are also referred to as collapsars