Quasi periodic oscillations in black hole binaries

S. E. Motta

doi:10.1002/asna.201612320

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arXiv · 1603.07885

Quasi periodic oscillations in black hole binaries

S. E. Motta

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Abstract

Fast time variability is the most prominent characteristic of accreting systems and the presence of quasi periodic oscillations (QPOs) is a constant in all accreting systems, from cataclysmic variables to AGNs, passing through black hole and neutron star X-ray binaries and through the enigmatic ultra-luminous X-ray sources. In this paper I will briefly review the current knowledge of QPOs in black hole X-ray binaries, mainly focussing on their observed properties, but also mentioning the most important models that have been proposed to explain the origin of QPOs over the last decades.

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S. E. Motta. 2016-03-25. Quasi periodic oscillations in black hole binaries. https://doi.org/10.1002/asna.201612320

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