QPOs from Radial and Vertical Oscillation of Shocks in Advective Accretion Flows
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🌌 astro-ph
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advectiveflowsqposaccretionbreakcomputedcoolingcurve
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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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