Physics
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002basi...30..317a&link_type=abstract
Bulletin of the Astronomical Society of India, Vol.30, p. 317-320
Physics
Accretion, Accretion Disks, Black Hole Physics, Hydrodynamics, Shock Waves
Scientific paper
We identify a new type of instability of the accrelation flow which is formed due to interaction of the outgoing winds with the incoming flow. Mainly due to shear instability, the flow oscillates around the equatorial plane. We show that in the shocks are formed in accretion flows, this new type of oscillation persists along with the usual radial oscillation.
Acharya K.
Chakrabarti Sandip K.
Molteni Diego
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