KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK and Gabriel TÖRÖK. Multi-resonance orbital model of HF QPOs. In Proceedings of the International Astronomical Union, Symposium No. 290: Feeding compact objects: Accretion on all scales. Cambridge, UK: Cambridge University Press, 2013, p. 315-316. ISBN 978-1-107-03379-5. Available from: https://dx.doi.org/10.1017/S1743921312020182.
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Basic information
Original name Multi-resonance orbital model of HF QPOs
Authors KOTRLOVÁ, Andrea, Zdeněk STUCHLÍK and Gabriel TÖRÖK.
Edition Cambridge, UK, Proceedings of the International Astronomical Union, Symposium No. 290: Feeding compact objects: Accretion on all scales, p. 315-316, 2 pp. 2013.
Publisher Cambridge University Press
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW URL
Organization unit Faculty of Philosophy and Science in Opava
ISBN 978-1-107-03379-5
ISSN 1743-9221
Doi http://dx.doi.org/10.1017/S1743921312020182
Keywords in English accretion; accretion disks; X-rays: binaries; black hole physics
Tags , GA202-090772, sbornik
Tags International impact
Links GA202/09/0772, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 7/4/2021 15:02.
Abstract
Using known frequencies of the twin peak high-frequency quasiperiodic oscillations (HF QPOs) and known mass M of the central black hole, the black-hole dimensionless spin a can be determined assuming a concrete version of the resonance model. However, large range of observationally limited values of the black hole mass implies a low precision of the spin estimates. We discuss the possibility of higher precision of the black hole spin a measurements in the framework of multi-resonance model inspired by observations of more than two HF QPOs in some black hole sources. We determine the spin and mass dependence of the twin peak frequencies with a general rational ratio n:m assuming a non-linear resonance of oscillations with the epicyclic and Keplerian frequencies or their combinations. In the multi-resonant model, the twin peak resonances are combined properly to give the observed frequency set. We focus on the special case of duplex frequencies, when the top, bottom, or mixed frequency i
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