Das, Tapas K.2012-03-142012-03-142001-07-02http://hdl.handle.net/11007/1482Using two different pseudo-Schwarzschild potentials proposed by Artemova et. al, 1 we formulate and solve the equations governing spherically symmetric transonic inflow and outflow in presence of a relativistic hadronic pressure mediated steady, standing, spher- ical shock around the central compact object and then we self-consistently connect the accretion-wind solutions to calculate the mass outflow rate R ˙ m in terms of minimum number of flow parameters. Also we study the dependence of this rate on various bound- ary conditions governing the flow.enPseudo-Schwarzschild descriptionCcretion-powered spherical outflowArticle