BAKALA, Pavel, Petr ČECH, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK and Martin URBANEC. Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model. Astronomy & Astrophysics. FR - Francouzská republika, 2010, vol. 522, A72, 7 pp. ISSN 0004-6361. Available from: https://dx.doi.org/10.1051/0004-6361/201014731.
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Basic information
Original name Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model
Authors BAKALA, Pavel, Petr ČECH, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ, Gabriel TÖRÖK and Martin URBANEC.
Edition Astronomy & Astrophysics, FR - Francouzská republika, 2010, 0004-6361.
Other information
Original language English
Type of outcome Article in a journal
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
Doi http://dx.doi.org/10.1051/0004-6361/201014731
UT WoS 000284153100078
Keywords in English QUASI-PERIODIC OSCILLATIONS, HIGH-FREQUENCY QPOS, X-RAY BINARIES, INTEGRATED RELATIVISTIC TORI, EQUATION-OF-STATE, SOURCE 4U 1636-53, BLACK-HOLE SPIN, KHZ QPOS, KILOHERTZ QPOS, SLENDER TORI
Tags , GA202-090772, LC06014, MSM4781305903
Tags International impact, Reviewed
Links GA202/09/0772, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 7/12/2020 12:05.
Abstract
The high-frequency quasi-periodic oscillations (HF QPOs) that appear in the X-ray fluxes of low-mass X-ray binaries remain an unexplained phenomenon. Among other ideas, it has been suggested that a non-linear resonance between two oscillation modes in anaccretion disc orbiting either a black hole or a neutron star plays a role in exciting the observed modulation. Several possible resonances have been discussed. A particular model assumes resonances in which the disc-oscillation modes have the eigenfrequencies equal to the radial and vertical epicyclic frequencies of geodesic orbital motion. This model has been discussed for black hole microquasar sources as well as for a group of neutron star sources.
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