Detailed Information on Publication Record
2007
Reverse of twin peak kHz QPO interrelationship in the six atoll sources
ČERMÁK, Petr, Zdeněk STUCHLÍK and Gabriel TÖRÖKBasic information
Original name
Reverse of twin peak kHz QPO interrelationship in the six atoll sources
Authors
Edition
Opava, Proceedings of RAGtime 8/9: Workshops on black holes and neutron stars, p. 511-522, 11 pp. 2007
Publisher
Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, 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
Organization unit
Faculty of Philosophy and Science in Opava
ISBN
978-80-7248-419-5
Keywords in English
X rays, binaries, neutron stars, accretion discs
Tags
Tags
International impact
Links
LC06014, research and development project. MSM4781305903, plan (intention).
Změněno: 3/12/2020 13:51, Mgr. Pavlína Jalůvková
Abstract
V originále
For six neutron star atoll sources spanning wide range of frequencies we investigate whether the relationship between the rms amplitudes and quality factors of the observed kHzQPO LU display features that could have a significant meaning in terms of theproposed QPO models.We find for all the six sources that after the twin kHz QPOs pass a point (or the narrow interval) where their ratio R equals 1:5 the lower/upper oscillation becomes stronger/weakerthan other one with increasing QPO frequency. Existence of a similar effect close to R D 1:33 or R D 1:25 is also indicated. This interval lies between frequencies corresponding to 3=2 and 4=3 (or 5=4) frequency ratio. This finding implies restrictions to the orbital QPO models (both hot spot- and disc oscillations- like) and also to QPO modulation mechanism. In a wider context, our results may indicate the existence of an energy over flow between the upper and lower QPO mode when their ratio is close to ratio of small integral numbers.