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 a Włodek KLUŹNIAK

Základní údaje

Originální název

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

Autoři

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

Vydání

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

Nakladatel

American Institute of Physics

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-0-7354-0359-8

DOI

https://doi.org/10.1063/1.2399658

EID Scopus

2-s2.0-77956661436

Klíčová slova anglicky

Relativity and gravitation, X-ray binaries, time variability

Štítky

FÚ, MSM4781305903, sbornik

Příznaky

Mezinárodní význam

Návaznosti

MSM4781305903, záměr.

Změněno: 3. 12. 2020 13:39, Mgr. Pavlína Jalůvková

Anotace

V originále

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.

Citovat

ABRAMOWICZ, Marek; Zdeněk STUCHLÍK; Gabriel TÖRÖK a 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, s. "A33"-"A33", 1 s. ISBN 978-0-7354-0359-8. Dostupné z: 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 a 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, s.~''A33''-''A33'', 1 s. ISBN~978-0-7354-0359-8. Dostupné z: https://doi.org/10.1063/1.2399658.

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