The Twin Peak QPOs in Neutron Star and Black Hole Sources: What is explained, and What is not

Details The Twin Peak QPOs in Neutron Star and Black Hole Sources: What is explained, and What is not The Twin Peak QPOs in Neutron Star and Black Hole Sources: What is explained, and What is not

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007rmxac..27....8a&link_type=abstract

Triggering Relativistic Jets (Eds. William H. Lee & Enrico Ramírez-Ruiz) Revista Mexicana de Astronomía y Astrofísica (Serie de

Physics

3

Accretion, Accretion Disks, Black Hole Physics, Hydrodynamics, Stars: Neutron

Scientific paper

The resonance model proposed in 2000 by Kluzniak and Abra-mo-wicz, explains the twin peak, high frequency, quasi periodic oscillations (HF QPOs) observed in the X-ray flux from black hole and neutron stars, as a non-linear resonance in modes of oscillations of accretion flows in strong gravity. While several important physical questions remain unanswered, recent observations of HF QPOs provide direct evidence of non-linear resonances. This article gives an up to date (May 2006) review of what has been explained, and what has not been explained, by the resonance model.

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