A non-linear resonance model for the black hole and neutron
star QPOs: theory supported by observations

D 2006

A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations

ABRAMOWICZ, Marek; Zdeněk STUCHLÍK; Gabriel TÖRÖK and Włodek KLUŹNIAK

Basic information

Original name

A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations

Authors

ABRAMOWICZ, Marek; Zdeněk STUCHLÍK; Gabriel TÖRÖK and Włodek KLUŹNIAK

Edition

United States of America, Albert Einstein Century International Conference, p. "A33"-"A33", 1 pp. 2006

Publisher

American Institute of Physics

Other information

Language

English

Type of outcome

Proceedings paper

Field of Study

10308 Astronomy

Confidentiality degree

is not subject to a state or trade secret

Organization unit

Faculty of Philosophy and Science in Opava

ISBN

978-0-7354-0359-8

DOI

https://doi.org/10.1063/1.2399658

EID Scopus

2-s2.0-77956661436

Keywords in English

Relativity and gravitation, X-ray binaries, time variability

Links

MSM4781305903, plan (intention).

Changed: 3/12/2020 13:39, Mgr. Pavlína Jalůvková

Abstract

In the original language

Kilohertz Quasi-Periodic Oscillations (QPOs) have been detected in many accreting X-ray binaries. It has been suggested that the highest QPO frequencies observed in the modulation of the X-ray flux reflect a non-linear resonance between two modes of accreting disk oscillation. This hypothesis implies certain very general predictions, several of which have been borne out by observations. Some of these follow from properties of non-linear oscillators, while the others are specific to oscillations of fluidin strong gravity. A 3:2 resonant ratio of frequencies can be clearly recognized in the black-hole as well as in the neutron-star QPO data.

Cite

ABRAMOWICZ, Marek; Zdeněk STUCHLÍK; Gabriel TÖRÖK and Włodek KLUŹNIAK. A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations. In Albert Einstein Century International Conference. United States of America: American Institute of Physics, 2006, p. "A33"-"A33", 1 pp. ISBN 978-0-7354-0359-8. Available from: https://doi.org/10.1063/1.2399658.

@inproceedings{42200,
   author = {Abramowicz, Marek and Stuchlík, Zdeněk and Török, Gabriel and KLUŹNIAK, Włodek},
   address = {United States of America},
   booktitle = {Albert Einstein Century International Conference},
   doi = {https://doi.org/10.1063/1.2399658},
   keywords = {Relativity and gravitation, X-ray binaries, time variability},
   language = {eng},
   location = {United States of America},
   isbn = {978-0-7354-0359-8},
   pages = {"A33"-"A33"},
   publisher = {American Institute of Physics},
   title = {A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations},
   year = {2006}
}

TY  - CONF
ID  - 42200
AU  - Abramowicz, Marek - Stuchlík, Zdeněk - Török, Gabriel - KLUŹNIAK, Włodek
PY  - 2006
TI  - A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations
PB  - American Institute of Physics
CY  - United States of America
SN  - 9780735403598
KW  - Relativity and gravitation, X-ray binaries, time variability
N2  - Kilohertz Quasi-Periodic Oscillations (QPOs) have been detected in many accreting X-ray binaries. It has been suggested that the highest QPO frequencies observed in the modulation of the X-ray flux reflect a non-linear resonance between two modes of accreting disk oscillation. This hypothesis implies certain very general predictions, several of which have been borne out by observations. Some of these follow from properties of non-linear oscillators, while the others are specific to oscillations of fluidin strong gravity. A 3:2 resonant ratio of frequencies can be clearly recognized in the black-hole as well as in the neutron-star QPO data.
ER  -

ABRAMOWICZ, Marek; Zdeněk STUCHLÍK; Gabriel TÖRÖK and Włodek KLU$\backslash$'ZNIAK. A non-linear resonance model for the black hole and neutron star QPOs: theory supported by observations. In \textit{Albert Einstein Century International Conference}. United States of America: American Institute of Physics, 2006, p.~''A33''-''A33'', 1 pp. ISBN~978-0-7354-0359-8. Available from: https://doi.org/10.1063/1.2399658.

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