J 2007

A remark about possible unity of the neutron star and black hole high frequency QPOs

TÖRÖK, Gabriel, Zdeněk STUCHLÍK and Pavel BAKALA

Basic 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

Článek v odborném periodiku

Confidentiality degree

není předmětem státního či obchodního tajemství

Organization unit

Faculty of Philosophy and Science in Opava

DOI

http://dx.doi.org/10.2478/s11534-007-0039-0

UT WoS

000251320600001

Keywords in English

X-rays; binaries; accretion; accretion discs; stars; neutron

Tags

clanek, Torokcentrum

Tags

International impact, Reviewed
Změněno: 12/4/2021 14:17, RNDr. Kateřina Klimovičová, Ph.D.

Abstract

V originále

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.
Displayed: 27/12/2024 08:05