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• W1984499367 abstract "Recent hydrodynamical simulations of radiatively inefficient black hole accretion flows with low viscosity have demonstrated that these flows differ significantly from those described by an advection-dominated model. The black hole flows are advection-dominated only in their inner parts but convectively dominated at radii R 102RG. In such flows, the radiative output comes mostly from the convection part, and the radiative efficiency is independent of accretion rate and equals BH 10-3. This value gives a limit for how dim an accreting black hole could be. It agrees with recent Chandra observations, which indicate that accreting black holes in low-mass X-ray binaries are dimmer by a factor of about 100 than neutron stars accreting with the same accretion rates." @default.
• W1984499367 created "2016-06-24" @default.
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• W1984499367 date "2001-06-10" @default.
• W1984499367 modified "2023-10-16" @default.
• W1984499367 title "How Dim Could Accreting Black Holes Be?" @default.
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• W1984499367 doi "https://doi.org/10.1086/320933" @default.
• W1984499367 hasPublicationYear "2001" @default.
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