  We present solutions to the accretion disk structure equations in which
advective cooling is accounted for in a self-consistent way. It is shown that
for high rates of accretion, above a critical value, when without advection
there are no solutions extending continuously from large to small radii, there
exist global solutions with self-consistent advective cooling. These solutions
are quite different fromthose solutions obtained earlier by other authors,
where advective cooling was not treated self-consistently.
