Аннотация:The galactic microquasar SS 433 is a super-critically accreting black hole candidate and their
relativistic jets have been interpreted to originate in the acceleration by the radiation pressure in
the inner accretion disk. Based on the initial 1D models of supercritical accretion disk with mass
loss and advection, we examine the disk and jets of SS 433 with dotM 10^3 dot M crit
by two-dimensional radiation hydrodynamical calculations. ...