Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
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DOI: 10.1093/mnras/staa1338
Abstract: Coalescence of intermediate-mass black holes (IMBHs) as a result of the migration toward galactic centers via dynamical friction may contribute to the formation of supermassive BHs. Here we reinvestigate the gaseous dynamical friction, which was… read more here.
Keywords: black holes; intermediate mass; gaseous dynamical; mass black ... See more keywords