QPOs from Radial and Vertical Oscillation of Shocks in Advective Accretion Flows

Details QPOs from Radial and Vertical Oscillation of Shocks in Advective Accretion Flows QPOs from Radial and Vertical Oscillation of Shocks in Advective Accretion Flows

2005-01-14

arxiv.org/abs/astro-ph/0501293v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures To be published in the Proceedings of 10th Marcel Grossman Meeting, Ed. R. Ruffini et al. (World Scientific

Scientific paper

We present results of several numerical simulations of two dimensional
advective flows which include cooling processes. We show that the computed
light curve is similar to the $\chi$ state in GRS 1915+105. The power density
spectrum (PDS) also shows presence of QPOs near the break frequency.

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