6533b851fe1ef96bd12a9a44
RESEARCH PRODUCT
Radiative 2D Shocks, Super-Eddington Disks and Jets around Black Holes
V. TeresiDiego MolteniElena ToscanoToru Okudasubject
Shock wavePhysicsGeneral Relativity and Quantum CosmologyBinary black holeIntermediate-mass black holeAstrophysics::High Energy Astrophysical PhenomenaRadiative transferStellar black holeAstrophysicsSpin-flipAstrophysics::Galaxy AstrophysicsGamma-ray burst progenitorsAccretion (astrophysics)description
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.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2005-01-01 | AIP Conference Proceedings |