Computation of Mass-Outflow Rates From Advective Accretion Disks Around   Black Holes
  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). 
Tapas K. Das (S.N. Bose National Centre for Basic Sciences, Salt Lake,   Calcutta)