Radiative 2D Shocks, Super-Eddington Disks and Jets around Black Holes

Details Radiative 2D Shocks, Super-Eddington Disks and Jets around Black Holes Radiative 2D Shocks, Super-Eddington Disks and Jets around Black Holes

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..395o&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 395-396 (2005).

Astronomy and Astrophysics

Astrophysics

1

Black Holes, Shock Waves, Accretion Disks, Black Holes

Scientific paper

It is well known that rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the centrifugal force. Such shock waves in 2D accretion flows are examined by 2D radiation hydrodynamical calculations. We also examine super-Eddington accretion disks with 15 ṀE around black holes, focusing on a small collimation degree of the jet and a large mass-outflow rate observed in the X-ray source SS 433.

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