Shock waves and QPOs in 2D rotating accretion flows around black holes

Details Shock waves and QPOs in 2D rotating accretion flows around black holes Shock waves and QPOs in 2D rotating accretion flows around black holes

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..417o&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

Planetary Bow Shocks, Interplanetary Shocks, Black Holes, Masses, Accretion And Accretion Disks, Pulsations, Oscillations, And Stellar Seismology

Scientific paper

We examine numerically shock waves formed in 2D rotating accretion flows around a stellar-mass and a supermassive black holes, while taking account of the cooling and heating of the gas and the radiation transport. As the results, we obtain general properties of the shock oscillations and the luminosity behaviors as QPOs independent of the black hole masses.

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