Detailed Information on Publication Record
2007
The twin peak QPOs in neutron star and black hole
TÖRÖK, GabrielBasic information
Original name
The twin peak QPOs in neutron star and black hole
Authors
Edition
Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), MX - Spojené státy mexické, 2007, 0185-1101
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Confidentiality degree
není předmětem státního či obchodního tajemství
Organization unit
Faculty of Philosophy and Science in Opava
Keywords in English
Accretion discs, Black hole physics, hydrodynamics, neutron stars
Tags
Tags
International impact, Reviewed
Links
MSM4781305903, plan (intention).
Změněno: 6/4/2021 11:35, Mgr. Pavlína Jalůvková
Abstract
V originále
The resonance model proposed in 2000 by Kluzniak and Abramowicz, explains the twin peak, high frequency, quasi periodic oscillations (HF QPOs) observed in the X-ray flux from black hole and neutron stars, as a non-linear resonance in modes of oscillations of accretion flows in strong gravity. While several important physical questions remain unanswered, recent observations of HF QPOs provide direct evidence of non-linear resonances. This article gives an up to date (May 2006) review of what has been explained, and what has not been explained, by the resonance model.