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The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries
Zhang, CM; Yin, HX; Zhao, YH; Zhang, F; Song, LM; Zhang F(张帆); Song LM(宋黎明)
2006
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷号366期号:4页码:1373-1377
通讯作者Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China ; Chinese Acad Sci, Inst High Energy Phys, Inst Astron, Beijing 100039, Peoples R China
文章类型Article
摘要We analyzed the recently published kHz quasi-period oscillaiton (QPO) data in the neutron star low-mass X-ray binaries (LMXBs), in order to investigate the different correlations of the twin-peak kHz QPOs in bright Z sources and in the less luminous Atoll sources. We find a power-law relation nu(1)similar to nu(b)(2) between the upper and the lower kHz QPOs with different indices: b similar or equal to 1.5 for the Atoll source 4U 1728-34 and b similar or equal to 1.9 for the Z source Sco X-1. The implications of our results for the theoretical models for kHz QPOs are discussed.
关键词accretion, accretion discs binaries : close stars : neutron X-rays : stars
学科领域Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics ; Astronomy & Astrophysics
DOI10.1111/j.1365-2966.2006.09920.x
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语种英语
研究领域[WOS]Astronomy & Astrophysics ; Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000235696500018
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被引频次:51[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/239319
专题粒子天体物理中心
作者单位中国科学院高能物理研究所
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Zhang, CM,Yin, HX,Zhao, YH,et al. The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2006,366(4):1373-1377.
APA Zhang, CM.,Yin, HX.,Zhao, YH.,Zhang, F.,Song, LM.,...&宋黎明.(2006).The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,366(4),1373-1377.
MLA Zhang, CM,et al."The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 366.4(2006):1373-1377.
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