Spectral and Timing Properties of Magnetized Advective Flows with Standing Shocks

Details Spectral and Timing Properties of Magnetized Advective Flows with Standing Shocks Spectral and Timing Properties of Magnetized Advective Flows with Standing Shocks

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1130m&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

Advective flows are known to have standing, oscillating or propagating shocks in the disk which are responsible for the quasi-periodic oscillations. We have calculated the QPO frequency from shock locations (xs) in presence of cooling effects. We have shown the change in the ratio of total integrated power (high/low) with shock location as well as with the accretion rates. These results generally agree with observations.

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