2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/10297We 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.9 pages, 4 figures, tarred and gzipped. Uses aasms4.styAstrophysicstext