Computation of Mass-Outflow Rates From Advective Accretion Disks Around Black Holes
Preprint
- 10 July 1998
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).Keywords
All Related Versions
- Version 1, 1998-07-10, ArXiv
- Published version: , 113.
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