Non-linear resonances in accretion disks and QPOs

Details Non-linear resonances in accretion disks and QPOs Non-linear resonances in accretion disks and QPOs

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..128k&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Physics

1

Black Hole Physics, Stars: Neutron, X-Rays: Binaries

Scientific paper

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.

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