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A global study of type B quasi-periodic oscillation in black hole X-ray binaries
Gao HQ(高汉秦); Chen YP(陈玉鹏); Zhang Z(张镇); Zhang SN(张双南); Zhang S(张澍); Ma X(马想); Li ZJ(李子健); Qu JL(屈进禄); Gao, HQ; Zhang, L; Chen, YP; Zhang, Z; Chen, L; Zhang, SN; Zhang, S; Ma, X; Li, ZJ; Bu, QC; Qu, JL
2017
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
EISSN1365-2966
Volume466Issue:1Pages:564-573
SubtypeArticle
AbstractWe performed a global study on the timing and spectral properties of type-B quasi-periodic oscillations (QPOs) in the outbursts of black hole X-ray binaries. The sample is built based on the observations of Rossi X-ray Timing Explorer (RXTE), via searching in the literature in RXTE era for all the identified type-B QPOs. To enlarge the sample, we also investigated some type-B QPOs that are reported but not yet fully identified. Regarding to the time lag and hard/soft flux ratio, we found that the sources with type-B QPOs behave in two subgroups. In one subgroup, type-B QPO shows a hard time lag that first decreases and then reverse into a soft time lag along with softening of the energy spectrum. In the other subgroup, type-B QPOs distribute only in a small region with hard time lag and relatively soft hardness. These findings may be understood with a diversity of the homogeneity showing up for the hot inner flow of different sources. We confirm the universality of a positive relation between the type-B QPO frequency and the hard component luminosity in different sources. We explain the results by considering that the type-B QPO photons are produced in the inner accretion flow around the central black hole, under a local Eddington limit. Using this relationship, we derived a mass estimation of 9.3-27.1 M-circle dot for the black hole in H 1743-322.
Keywordaccretion, accretion discs black hole physics stars: oscillations X-rays: binaries
DOI10.1093/mnras/stw3146
WOS KeywordLOW-FREQUENCY OSCILLATIONS ; TRANSIENT XTE J1859+226 ; GRS 1915+105 ; ACCRETION DISCS ; LOW/HARD STATE ; CYGNUS X-1 ; PHASE-LAG ; GX 339-4 ; OUTBURST EVOLUTION ; ENERGY-DEPENDENCE
Indexed BySCI ; SCOPUS ; ADS
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000398112400039
ADS Bibcode2017MNRAS.466..564G
ADS URLhttps://ui.adsabs.harvard.edu/abs/2017MNRAS.466..564G
ADS CITATIONShttps://ui.adsabs.harvard.edu/abs/2017MNRAS.466..564G/citations
AXRIV CODE171
inspireid1509493
Citation statistics
Cited Times:7 [INSPIRE]
Cited Times:9 [ADS]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/284849
Collection粒子天体物理中心
理论物理室
Affiliation中国科学院高能物理研究所
First Author AffilicationInstitute of High Energy
Recommended Citation
GB/T 7714
Gao HQ,Chen YP,Zhang Z,et al. A global study of type B quasi-periodic oscillation in black hole X-ray binaries[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,466(1):564-573.
APA 高汉秦.,陈玉鹏.,张镇.,张双南.,张澍.,...&Qu, JL.(2017).A global study of type B quasi-periodic oscillation in black hole X-ray binaries.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,466(1),564-573.
MLA 高汉秦,et al."A global study of type B quasi-periodic oscillation in black hole X-ray binaries".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 466.1(2017):564-573.
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