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- W2007224059 abstract "We investigate the process of steady-state spherical accretion onto black holes when the infalling gas is optically thick to the outgoing radiation. The transfer of radiation is treated in the diffusion approximation, and the calculation is done relativistically so that the region near the Schwarzschild radius may be included. The luminosity is taken as a free parameter. It is found that, in cases of sufficiently high luminosity and mass flux, a radiation-broadened shock must form and prevent steady supersonic flow through the Schwarzschild radius. Fluctuations on time scales of microseconds to milliseconds could result." @default.
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- W2007224059 date "1980-08-01" @default.
- W2007224059 modified "2023-09-27" @default.
- W2007224059 title "Relativistic accretion - The optically thick case" @default.
- W2007224059 doi "https://doi.org/10.1086/158227" @default.
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