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On the origin of the low-frequency QPO in GRS 1915+105 rho state
Yan, Shu-Ping1,2; Wang, Na1; Ding, Guo-Qiang1
2013-02-21
Conference NameIAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years
Source PublicationNeutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291
Volume291
Pages565-567
Conference Date20-31 August 2012
Correspondent Emailyanshup@xao.ac.cn ; na.wang@xao.ac.cn ; dinggq@xao.ac.cn
Conference PlaceBeijing, China
PublisherCambridge University Press
Project Number2009CB824800 ; KJCX2-YW-T09 ; 200821164 ; LHXZ 200802
AbstractWe performed a phase-resolved timing analysis of GRS 1915+105 in its rho state and identify detailed rho cycle evolution of frequency, amplitude and coherence of the low-frequency quasi-periodic oscillation (LFQPO). We combined our timing results with the spectral study by Neilsen et al. (2011) to do an elaborate contrast analysis. The results are naturally explained by tying the LFQPO to the corona.
Funding OrganizationIAU ; IAU ; IAU ; IAU
KeywordAccretion Accretion Disks Oscillations Grs 1915+105
DOI10.1017/S1743921312024891
URL查看原文
Language英语
ISBN978-1-107-03380-1
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Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/989
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
其它
Corresponding AuthorYan, Shu-Ping; Wang, Na; Ding, Guo-Qiang
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150, Science 1-Street, Urumqi, Xinjiang 830011, China
2.University of Chinese Academy of Sciences, 19A Yuquan road, Beijing 100049, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Yan, Shu-Ping,Wang, Na,Ding, Guo-Qiang. On the origin of the low-frequency QPO in GRS 1915+105 rho state[C]:Cambridge University Press,2013:565-567.
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