Fig. 4 from Resonance in Forced Oscillations of an Accretion Disk and Kilohertz Quasi‐periodic Oscillations

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Resonance in Forced Oscillations of an Accretion Disk and Kilohertz Quasi‐periodic Oscillations

Authors: William H. Lee, Marek A. Abramowicz, and Włodek Kluźniak

Lee, Abramowicz, & Kluźniak 2004 The Astrophysical Journal Letters 603 L93.

Provider: AAS Journals

Caption: Fig. 4.

Peak power in the vertical epicyclic oscillations induced in the torus by the periodic perturbation of Fig. 3, as a function of ﹩\nu _{s\,}/ ( \zeta _{0}-\kappa _{0}) ﹩. Three peaks at 1.0, 1.5, and 2.0 are clearly visible. For this calculation, ﹩\nu _{s}﹩, the pulsar perturbation frequency, varied while ﹩\zeta _{0}-\kappa _{0}﹩ was held fixed at 200 Hz.

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