Abstract
Using 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, spherical shock around the central compact object. Then we self-consistently connect the accretion-wind solutions to calculate the mass outflow rate [Formula: see text] in terms of a minimum number of flow parameters. We also study the dependence of this rate on various boundary conditions governing the flow.
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