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Two component advective flows are the most physical accretion disks whicharise from theoretical consideration. Since viscosity is the determiningfactor, we investigate the effects of viscous stresses on accretion flowsaround a nonrotating black hole. As a consequence of angular momentum transferby viscosity in an accretion flow, the angular momentum distribution ismodified. We include cooling effects and found that a Keplerian disk isproduced on the equatorial plane and the flow above and below remains subKeplerian. This gives a complete picture to date, of the formation of a Twocomponent advective flow around a black hole.

Numerical Simulations of a Two Component Advective Flow for The Study of the Spectral and Timing Properties of Black Holes