Computation of Mass-Outflow Rates From Advective Accretion Disks Around Black Holes
classification
🌌 astro-ph
gr-qc
keywords
advectivemassaccretionagreesaroundastro-phbarrierblack
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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).
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