KOTRLOVÁ, Andrea, Gabriel TÖRÖK and Zdeněk STUCHLÍK. Multi-resonance models of QPOs. In Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2007, p. 363-416, 53 pp. ISBN 978-80-7248-419-5.
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Basic information
Original name Multi-resonance models of QPOs
Authors KOTRLOVÁ, Andrea, Gabriel TÖRÖK and Zdeněk STUCHLÍK.
Edition Opava, Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars, p. 363-416, 53 pp. 2007.
Publisher Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher Czech Republic
Confidentiality degree is not subject to a state or trade secret
Organization unit Faculty of Philosophy and Science in Opava
ISBN 978-80-7248-419-5
Keywords in English compact objects, X-ray variability, theory, observations
Tags , GD205-03H144, LC06014, MSM4781305903, RAGtime, sbornik
Tags International impact
Links GD205/03/H144, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 3/12/2020 14:22.
Abstract
In the simple orbital resonance models we determine the spin and mass dependence of the twin peak frequencies for non-linear resonances of oscillations with the epicyclic and Keplerian frequencies or their combinations in the case of a general rational frequency ratio n:m, n > m. In the multi-resonant model, the twin peak resonances are combined properly to give the observed frequency set. In the first one, related probably to the neutron star binary systems, more instances of one resonance occur at more specific radii. In the second case, more resonances are sharing one specific radius, allowing for "cooperative" resonant phenomena in the field of black holes with a specific value of spin. In the third ("ugly") case, more resonances occur at more specific radii; we restrict our attention to the case of two such resonant radii.
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