KMS of Xinjiang Astronomical Observatory, CAS
| A statistical study on the low-frequency quasi-periodic oscillation amplitude spectrum and amplitude in GRS 1915+105 | |
Yan, Shu-Ping1,2 ; Ding, Guo-Qiang1; Wang, Na1; Qu, Jin-Lu3; Song, Li-Ming3
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| 2013-09-01 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| Volume | 434Issue:1Pages:59-68 |
| Contribution Rank | 1 |
| Abstract | A statistical study was made on both the energy dependence of the low-frequency quasi-periodic oscillation (QPO) amplitude (LFQPO amplitude spectrum) and the LFQPO amplitude from all the RXTE observations of GRS 1915+105. Based on the two-branch correlation of the LFQPO frequency and the hardness ratio, the observations that were suitable for evaluating the LFQPO amplitude spectrum were divided into two groups. According to a comparison between the radio and X-ray emissions, we deduced that the jets during the two groups of observations are very different. A negative correlation between the LFQPO frequency and the radio flux was found for one group. The LFQPO amplitude spectrum was fitted by a power law with an exponential cutoff in order to describe it quantitatively. It reveals that as the LFQPO frequency increases, the power law hardens. Furthermore, the cutoff energy first decreases, and then smoothly levels off. The fit also shows that the LFQPO amplitude spectra of the two groups are essentially the same, suggesting that the LFQPO does not originate from the jet. The LFQPO amplitude spectra are hard, indicating a possible origin of the LFQPO in the corona. As the LFQPO frequency increases, the LFQPO amplitude first increases and then decreases. The effects of the low-pass filter and the jet on the LFQPO amplitude are discussed. |
| Keyword | Black Hole Physics Accretion X-rays: Binaries Accretion Discs X-rays: Individual: Grs 1915+105 |
| Subtype | Article |
| WOS Headings | Science & Technology ; Physical Sciences |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | X-RAY BINARIES ; ACCRETION-EJECTION INSTABILITY ; LENS-THIRRING PRECESSION ; BLACK-HOLE CANDIDATES ; PHASE-LAG VARIABILITY ; RADIO-EMISSION ; RXTE OBSERVATIONS ; XTE J1550-564 ; TRANSIENT H1743-322 ; ENERGY-DEPENDENCE |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000323636800005 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/485 |
| 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 其它 |
| Corresponding Author | Yan, Shu-Ping; Wang, Na |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.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 | Yan, Shu-Ping,Ding, Guo-Qiang,Wang, Na,et al. A statistical study on the low-frequency quasi-periodic oscillation amplitude spectrum and amplitude in GRS 1915+105[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2013,434(1):59-68. |
| APA | Yan, Shu-Ping,Ding, Guo-Qiang,Wang, Na,Qu, Jin-Lu,&Song, Li-Ming.(2013).A statistical study on the low-frequency quasi-periodic oscillation amplitude spectrum and amplitude in GRS 1915+105.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,434(1),59-68. |
| MLA | Yan, Shu-Ping,et al."A statistical study on the low-frequency quasi-periodic oscillation amplitude spectrum and amplitude in GRS 1915+105".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 434.1(2013):59-68. |
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| A statistical study （767KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-ND | View Application Full Text | |
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