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• W3101578252 abstract "It is well known that rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the centrifugal force. We numerically examined such shock waves in 1D and 2D accretion flows, while taking account of the cooling and heating of the gas and the radiation transport. The numerical results show that the shock location shifts outward compared with that in adiabatic solutions, and that a more rarefied ambient density leads to a more outward shock location. In 2D-flow, we find an intermediate frequency QPO behavior of the shock location, as is observed in the black hole candidate GRS 1915|$+$|105." @default.
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• W3101578252 date "2004-06-25" @default.
• W3101578252 modified "2023-09-30" @default.
• W3101578252 title "Radiative Shocks in Rotating Accretion Flows around Black Holes" @default.
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• W3101578252 doi "https://doi.org/10.1093/pasj/56.3.547" @default.
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