Feeding supermassive black holes through supersonic turbulence and ballistic accretion
It has long been recognized that the main obstacle to the accretion of gas on to supermassive black holes (SMBHs) is a large specific angular momentum. It is feared that the gas settles in a large-scale disc, and that accretion would then proceed too inefficiently to explain the masses of the observ...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2011-06, Vol.413 (4), p.2633-2650 |
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