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Non-Linear Resonances in Accretion Disks and QPOs

Published online by Cambridge University Press:  22 February 2018

Włodek Kluźniak
Włodek Kluźniak*
Affiliation:
Institute of Astronomy, Zielona Góra University Copernicus Astronomical Center

Abstract

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Non-linear oscillations in the accretion disk are favored as an explanation of high-frequency QPOs observed in the light curves of low-mass X-ray binaries containing neutron stars, black holes, or white dwarfs.

Resumen

Resumen

Secundamos las oscilaciones no-lineales en el disco de acreción como una explicación de las “oscilaciones cuasi-periódicas” de alta frecuencia observadas en las curvas de luz de las binarias de rayos X de baja masa que contienen estrellas de neutrones, agujeros negros о enanas blancas.

Keywords

Black Hole Physics — StarsNeutron — X-RaysBinaries
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 128 - 129
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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