Open AccessOn the fate of gas accreting at a low rate on to a black hole
Author(s) -
Blandford Roger D.,
Begelman Mitchell C.
Publication year - 1999
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1999.02358.x
Subject(s) - physics , astrophysics , black hole (networking) , flux (metallurgy) , energy flux , accretion (finance) , radius , mechanics , astronomy , computer network , materials science , computer security , metallurgy , routing protocol , routing (electronic design automation) , computer science , link state routing protocol
Gas supplied conservatively to a black hole at rates well below the Eddington rate may not be able to radiate effectively and the net energy flux, including the energy transported by the viscous torque, is likely to be close to zero at all radii. This has the consequence that the gas accretes with positive energy so that it may escape. Accordingly, we propose that only a small fraction of the gas supplied actually falls on to the black hole, and that the binding energy it releases is transported radially outward by the torque so as to drive away the remainder in the form of a wind. This is a generalization of and an alternative to an `ADAF' solution. Some observational implications and possible ways to distinguish these two types of flow are briefly discussed.