出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要: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 ˙M =103 ˙Mc by two-dimensional
radiation hydrodynamical calculations. Depending on the viscosity parameter a, we obtain the
total luminosities more than 10 times higher than the Eddington luminosity, the jets mass-outflow
rates of 10
6 – 510
5Myr
1, and the wind mass-outflow rates of 10
6 – 10
4Myr
1,
which are generally compatible with the observed rates of SS 433. In addition, for a case of large
viscosity parameter a, we find a new type of instabilities of the accretion rates near the inner edge
and the disk luminosity. These instabilities grow into recurrent hot blobs which develop outward
and upward, and result in QPOs of the total luminosity with an amplitude of a factor 1 – 2 and
a quasi-period of 30 sec. This may explain a massive jet ejection and QPOs-like phenomena
observed recently in SS 433.