  We provide a 2.5-dimensional solution to a complete set of viscous
hydrodynamical equations describing accretion-induced outflow and then
plausible jet around black holes/compact objects. We prescribe a
self-consistent advective disk-outflow coupling model, which explicitly
includes the information of vertical flux. Inter-connecting dynamics of
inflow-outflow system essentially upholds the conservation laws. We provide a
set of analytical family of solutions through the self-similar approach. The
flow parameters of the disk-outflow system depend strongly on viscosity
parameter \alpha and cooling factor f.
