Point-wise Self-similar Solution for Spiral Shocks in an Accretion Disk with Mass Outflow in a Binary

We examine the properties of spiral shocks from a steady, adiabatic, non-axisymmetric accretion disk around compact star in binary. first time incorporate all possible influences binary through adopting Roche potential and Coriolis forces basic conservation equations. In this paper, we assume to be point-wise self-similar, flow is vertical hydrostatic equilibrium simplify study. also investigate mass outflow due shock compression apply it accreting white dwarf find that our model will beneficial overcome ad hoc assumption optically thick wind generally used studies progenitor supernovae Ia.