J 2007

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

BAKALA, Pavel, Zdeněk STUCHLÍK and Gabriel TÖRÖK

Basic information

Original name

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

Authors

Edition

CENTRAL EUROPEAN JOURNAL OF PHYSICS, DE - Spolková republika Německo, 2007, 1895-1082

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

UT WoS

000251320600001

Keywords in English

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

Tags

International impact, Reviewed

Links

GA202/06/0041, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Změněno: 14/12/2020 09:48, Mgr. Pavlína Jalůvková

Abstract

V originále

Series of papers discuss 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 rather exclude such a uniform origin. On the example of the atoll source 4U 1636-53 we illustrate that this is not neccesarily true.