Global transonic accretion and wind solutions for black hole flows with dΩ/dr viscosity and cooling are obtained by integrating the stiff angular momentum equation implicitly and the other equations explicitly.
Here,βis the inverse of plasma beta parameter and is used to find the magnitude of stochastic magnetic field required for computing the synchrotron emission
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Novel methodology to obtain transonic solutions for dissipative flows around compact objects
Global transonic accretion and wind solutions for black hole flows with dΩ/dr viscosity and cooling are obtained by integrating the stiff angular momentum equation implicitly and the other equations explicitly.