Computation of Mass-Outflow Rates From Advective Accretion Disks Around Black Holes
arXiv:astro-ph/9807105 · doi:10.1007/978-94-011-4750-7_8
Abstract
We self-consistently compute the mass outflow rate from a mass inflow using the conditions in the centrifugal barrier of an advective flow. Our detailed result agrees with the theoretical estimates given in Chakrabarti (1997; astro-ph/9801079).
10 Latex pages including figures. Kluwer Style files included. Appearing in `Observational Evidence for Black Holes in the Universe', ed. Sandip K. Chakrabarti, Kluwer Academic Publishers (DORDRECHT: Holland)