  Active galaxies and quasers are believed to harbour Black Holes at their
centers and at the same time produce cosmic radio jets through which immense
amount of matter and energy are ejected out of the core of the galaxy. In our
work we compute the mass outflow rates from advective accretion disks around
black holes, which, in principal could explain the origin of jet formation in
self-consistent manner. These computations are done using combinations of exact
transonic inflow and outflow solutions which may or may not form shock waves.
The approach of our calculation is somewhat different from that used in the
literature so far. Our work for the first time connects the accretion type and
wind type topologies self consistently. Our result, in general, matches with
numerical simulation works and successfully points out to non-steady behavior
which may evacuate the disk producing quiescene states.
