KMS of Xinjiang Astronomical Observatory, CAS
The energy dependence of the three types of low-frequency quasi-periodic oscillations in the black hole candidate H1743-322 | |
Li, Z. B.1![]() ![]() | |
2013-07-01 | |
Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
![]() |
Volume | 433Issue:1Pages:412-420 |
Contribution Rank | 1 |
Abstract | We investigate the properties of the centroid frequency of low-frequency quasi-periodic oscillation (LF QPOs, 0.1-30 Hz) during the 2003 outburst of H1743-322, by using the observational data of the Rossi X-ray Timing Explorer. We find that the frequency shows different energy dependences for each of the sub-classes of LF QPOs: the QPO frequency is proportional to photon energy for the type C QPOs while it is ambiguous for the type A and B QPOs. For type C QPOs, the slope of the frequency-energy relation versus frequency plot can be well described by a power law with frequency till similar to 7.5 Hz. Beyond similar to 7.5 Hz the slope goes down. The LF QPO amplitude decreases monotonically with the frequency for the type C but increases for the other two types. These properties provide a joint diagnostic for discriminating the different types of LF QPO. |
Keyword | Accretion Accretion Discs Black Hole Physics Stars: Individual: H1743-322 Stars: Low-mass Stars: Oscillations X-rays: Binaries |
Subtype | Article |
WOS Headings | Science & Technology ; Physical Sciences |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | X-RAY BINARIES ; XTE J1550-564 ; CENTROID FREQUENCY ; TIMING FEATURES ; SPECTRAL STATES ; GRS 1915+105 ; PHASE-LAG ; GX 339-4 ; BEHAVIOR ; ACCRETION |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000321461200034 |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/484 |
Collection | 已撤销研究室/团组_高能天体物理研究团组 |
Corresponding Author | Li, Z. B. |
Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Li, Z. B.,Zhang, S.,Qu, J. L.,et al. The energy dependence of the three types of low-frequency quasi-periodic oscillations in the black hole candidate H1743-322[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2013,433(1):412-420. |
APA | Li, Z. B..,Zhang, S..,Qu, J. L..,Gao, H. Q..,Zhao, H. H..,...&Song, L. M..(2013).The energy dependence of the three types of low-frequency quasi-periodic oscillations in the black hole candidate H1743-322.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,433(1),412-420. |
MLA | Li, Z. B.,et al."The energy dependence of the three types of low-frequency quasi-periodic oscillations in the black hole candidate H1743-322".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 433.1(2013):412-420. |
Files in This Item: | ||||||
File Name/Size | DocType | Version | Access | License | ||
The energy dependenc(852KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-ND | View Application Full Text |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment