Wind induced instabilities in accretion flow around black holes

Physics

Scientific paper

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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.

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