X-Ray Timing 2003: Rossi and Beyond

By P. Kaaret, F. Lamb, J. Swank. 2004

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Multi-resonance orbital model of high-frequency quasi-periodic oscillations: possible high-precision determination of black hole and neutron star spin (2013, background): “The standard orbital resonance model (Abramowicz & Kluźni ak 2001; Török et al. 2005; Aliev & Galtsov 1981) assumes nonlinear resonance between oscillation modes of an accretion disc orbiting a central object, here considered to be a rotating K err black hole (or a neutron star with exterior describ”
On the Origin of Radio Emission in the X-Ray States of XTE J1650–500 during the 2001-2002 Outburst (2004, background): “In that case, it is unlikely that an infrared re-flare would have been detected during the soft to hard state transition as in XTE J1550−564, GX 339−4 or 4U 1543−47 (Jain et al. 2001; Buxton & Bailyn 2003).”
Going with the Flow: Can the Base of Jets Subsume the Role of Compact Accretion Disk Coronae? (2005, methodology): “For a detailed discussion of these points, see the review article by Coppi (2004).”