2007
A remark about possible unity of the neutron star and black hole high frequency QPOs
TÖRÖK, Gabriel; Zdeněk STUCHLÍK and Pavel BAKALABasic information
Original name
A remark about possible unity of the neutron star and black hole high frequency QPOs
Authors
TÖRÖK, Gabriel; Zdeněk STUCHLÍK and Pavel BAKALA
Edition
CENTRAL EUROPEAN JOURNAL OF PHYSICS, WARSAW 41, VERSITA, 2007, 1895-1082
Other information
Language
English
Type of outcome
Article in a journal
Confidentiality degree
is not subject to a state or trade secret
Impact factor
Impact factor: 0.538
Organization unit
Faculty of Philosophy and Science in Opava
UT WoS
000251320600001
Keywords in English
X-rays; binaries; accretion; accretion discs; stars; neutron
Tags
Tags
International impact, Reviewed
Changed: 12/4/2021 14:17, RNDr. Kateřina Klimovičová, Ph.D.
Abstract
In the original language
In a series of papers it was discussed, on the basis of phenomenological arguments, whether the high frequency quasiperiodic oscillations (kHz QPOs) observed in the neutron-star and black-hole X-ray sources originate in the same physical mechanism. Recently it was suggested that a general trend seen in neutron star kHz QPOs instead excludes such a uniform origin. Using the example of the atoll source 4U 1636-53 we illustrate that this is not neccesarily true. (C) Versita Warsaw and Springer-Verlag Berlin Heidelberg. All rights reserved.