Super-Eddington slim accretion discs with winds
نویسندگان
چکیده
منابع مشابه
Super-Eddington black hole accretion: Polish doughnuts and slim disks
The theory of highly super-Eddington black hole accretion, Ṁ ≫ ṀEdd, was developed in the 1980s in Warsaw by Paczyński and his collaborators [1]–[9] in terms of Polish doughnuts , i.e. low viscosity, rotating accretion flows that are optically thick, radiation pressure supported, cooled by advection, and radiatively very inefficient. Polish doughnuts resemble fat tori with two narrow funnels al...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2011
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2011.18235.x