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The correlations between kHz and LF QPOs in the NSXBs
Li, Z. B.1; Wang, D. H.2
2013-02-21
Conference NameIAU Symposium 290:Feeding Compact Objects: Accretion on All Scales
Source PublicationFeeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium 290
Volume290
Pages261-262
Conference Date20 - 24 August 2012
Correspondent Emaillizhibing@xao.ac.cn
Conference PlaceBeijing, China
PublisherCambridge University Press
Project NumberXBBS201121 ; 11203064 ; 1143013 ; 11173024 ; 11173034
Contribution Rank1
Abstract

We study the correlations between low frequency (LF) and kHz quasi-periodic oscillations (QPOs) for 20 neutron star X-ray bianaries (NSXBs). We find that both upper and lower kHz QPOs correlate with the

Funding Organization西部之光 ; IAU ; 西部之光 ; IAU ; 西部之光 ; IAU ; 西部之光 ; IAU ; 国家自然科学基金 ; 国家自然科学基金 ; 国家自然科学基金 ; 国家自然科学基金
KeywordAccretion Stars: Neutron Stars: Oscillations X-rays: Binaries
DOI10.1017/S1743921312019916
URL查看原文
Language英语
ISBN978-1-107-03379-5
Citation statistics
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/981
Collection已撤销研究室/团组_高能天体物理研究团组
射电天文研究室
Corresponding AuthorLi, Z. B.
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150, Science 1-Street, Urumqi, Xinjiang, 830011, China
2.National Astronomical Observatories, Chinese Academy of Sciences, Bejing, 100012, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Li, Z. B.,Wang, D. H.. The correlations between kHz and LF QPOs in the NSXBs[C]:Cambridge University Press,2013:261-262.
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