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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

References

Abramowicz, M. A. & Kluźniak, W. 2003, in X-Ray Timing 2003: Rossi and Beyond, Kaaret, P., Swank, J., eds. in press, astro-ph/0312396Google Scholar
Abramowicz, M. A., Karas, V., Kluźniak, W. Lee, W., Rebusco, P. 2003 Publ. Astr. Soc. Japan., 55, 467 Google Scholar
Kluźniak, W., Abramowicz, M. A. 2000, Phys. Rev. Lett. (submitted), astro-ph/0105057Google Scholar
Kluźniak, W., Abramowicz, M. A. 2003, 12th Workshop on General Relativity and Gravitation, (Tokyo: Tokyo University Press), astro-ph/0304345Google Scholar
Kluźniak, W., Abramowicz, M. A., Kato, S., Lee, W., Stergioulas, N. 2003, ApJL in press, astro-ph/0308035Google Scholar
Kluźniak, W., Abramowicz, M. A., Lee, W. 2004, in X-Ray Timing 2003: Rossi and Beyond, Kaaret, P., Swank, J., eds in press, astro-ph/0402013Google Scholar
Lee, W.H., Abramowicz, M. A., Kluźniak, W. 2004. ApJLett. in pressGoogle Scholar
Mauche, C. 2002, ApJ 580, 423 Google Scholar
McClintock, J.E, Remillard, R. A. 2003, astro-ph/0306213 v.2Google Scholar
Psaltis, D., Belloni, T., van der Klis, M. 1999, ApJ 520, 262 Google Scholar
Rebusco, P. 2004, submittedGoogle Scholar
van der Klis, M., Wijnands, R.A.D., Home, K., Chen, W. 1997, ApJ 481, L97 Google Scholar
van der Klis, M. 2000, Ann. Rev. of A&A 38, 717 Google Scholar
Warner, B., astro-ph/0312182Google Scholar
Warner, B., Woudt, P.A., Pretorias, M.L. 2003, MNRAS 344, 1193 Google Scholar
Wijnands, R., van der Klis, M., Homan, J., Chakrabarty, D., Markwardt, С. B., Morgan, E. H. 2003 Nature, 6944, 44 Google Scholar