Radiatively Inefficient Accretion: Breezes, Winds and Hyperaccretion

Details Radiatively Inefficient Accretion: Breezes, Winds and Hyperaccretion Radiatively Inefficient Accretion: Breezes, Winds and Hyperaccretion

2011-10-24

arxiv.org/abs/1110.5356v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

13 pages, 8 figures, to appear in Monthly Notices of the Royal Astronomical Society

Scientific paper

We reformulate the adiabatic inflow-outflow (ADIOS) model for radiatively inefficient accretion flows, treating the inflow and outflow zones on an equal footing. For purely adiabatic flows (i.e., with no radiative losses), we show that the mass flux in each zone must satisfy Mdot ~ R^n with n=1, in contrast to previous work in which 0

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