Detailed Information on Publication Record
2017
A one-parametric formula relating the frequencies of twin-peak quasi-periodic oscillations
TÖRÖK, Gabriel, Kateřina GOLUCHOVÁ, Eva ŠRÁMKOVÁ, Jiří HORÁK, Pavel BAKALA et. al.Basic information
Original name
A one-parametric formula relating the frequencies of twin-peak quasi-periodic oscillations
Authors
TÖRÖK, Gabriel (203 Czech Republic, guarantor, belonging to the institution), Kateřina GOLUCHOVÁ (203 Czech Republic, belonging to the institution), Eva ŠRÁMKOVÁ (203 Czech Republic, belonging to the institution), Jiří HORÁK (203 Czech Republic), Pavel BAKALA (203 Czech Republic, belonging to the institution) and Martin URBANEC (203 Czech Republic, belonging to the institution)
Edition
1. vyd. Opava (Česká republika), Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic, p. 177-193, 17 pp. 2017
Publisher
Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Czech Republic
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
printed version "print"
References:
RIV identification code
RIV/47813059:19240/17:A0000038
Organization unit
Faculty of Philosophy and Science in Opava
ISBN
978-80-7510-256-0
ISSN
Keywords in English
X-rays: binaries; accretion; accretion disks; stars: neutron
Tags
International impact, Reviewed
Links
GA17-16287S, research and development project. LTI17018, research and development project.
Změněno: 6/4/2018 08:35, RNDr. Jan Hladík, Ph.D.
Abstract
V originále
Timing analysis of X-ray flux in more than a dozen low-mass X-ray binary systems containing a neutron star reveals remarkable correlations between frequencies of two characteristic peaks present in the power-density spectra. We find a simple analytic relation that well reproduces all these individual correlations. We link this relation to a physical model which involves accretion rate modulation caused by an oscillating torus.