KMS of Xinjiang Astronomical Observatory, CAS
| Spectral and Timing Analysis of the Black Hole Transient MAXI J1631–479 During its 2019 Outburst Observed with Insight-HXMT | |
| Fu,Yu-Cong1,2,3; Song,L. M.3; Ding,G. Q.1; Zhang,S. N.3; Qu,J. L.3; Zhang,S.3; Zhang,L.3; Bu,Q. C.4; Huang,Y.3; Ma,X.3; Yang,Z. X.2,3; Tuo,Y. L.3; Lu,X. F.3; Zhou,D. K.2,3; Wu,B. Y.2,3; Li,T. M.2,3; Xu,Y. C.2,3 | |
| 2022-10-12 | |
| Source Publication | Research in Astronomy and Astrophysics
 |
| ISSN | 1674-4527 |
| Volume | 22Issue:11 |
| Abstract | Abstract We report spectral and timing analysis of the black hole transient MAXI J1631–479 during the hard intermediate state of its 2019 outburst from the Insight-Hard X-ray Modulation Telescope (Insight-HXMT) observations. We find that the energy dependence of the type-C quasi-periodic oscillation (QPO) frequency evolves with time: during the initial rise of a small flare (～MJD 58526.0-58527.1), the QPO frequency increases with increasing energy from ～1 to ～100 keV, and then the frequency remains constant after MJD 58527.1. We discover a possible new phenomenon of Fe line’s QPO frequency jump that has never been observed for other black hole transients: during the small flare, the QPO frequency around the Fe line energy is higher than any other energy band, with the frequency difference Δf = 0.25 ± 0.08 Hz between 5.5–7.5 keV and other energy bands. The spectral analysis shows that the evolution of QPOs is related to the equivalent width of the narrow Fe line, and its equivalent width increases during this small flare. We propose that the QPO frequency difference results from the differential precession of a vertically extended jet, and the higher QPO frequency of Fe line could be caused by the layered jet when the jet scale increases. At the same time, the evolution of QPOs is related to the accretion rate, while the energy dependence of QPOs supports the existence of deceleration in the vertically distributed jet. |
| Corresponding Author | Fu,Yu-Cong() |
| Keyword | accretion accretion disks stars: black holes X-rays: binaries |
| DOI | 10.1088/1674-4527/ac8d80 |
| Language | 英语 |
| WOS ID | IOP:raa_22_11_115002 |
| Publisher | National Astromonical Observatories, CAS and IOP Publishing |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6194 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Fu,Yu-Cong |
| Affiliation | 1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, China; fuyucong@xao.ac.cn, dinggq@xao.ac.cn 2.University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China 3.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; songlm@ihep.ac.cn 4.Institut für Astronomie und Astrophysik, Kepler Center for Astro and Particle Physics, Eberhard Karls Universit?t, Sand 1, D-72076 Tübingen, Germany |
| 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 | Fu,Yu-Cong,Song,L. M.,Ding,G. Q.,等. Spectral and Timing Analysis of the Black Hole Transient MAXI J1631–479 During its 2019 Outburst Observed with Insight-HXMT[J]. Research in Astronomy and Astrophysics,2022,22(11). |
| APA | Fu,Yu-Cong.,Song,L. M..,Ding,G. Q..,Zhang,S. N..,Qu,J. L..,...&Xu,Y. C..(2022).Spectral and Timing Analysis of the Black Hole Transient MAXI J1631–479 During its 2019 Outburst Observed with Insight-HXMT.Research in Astronomy and Astrophysics,22(11). |
| MLA | Fu,Yu-Cong,et al."Spectral and Timing Analysis of the Black Hole Transient MAXI J1631–479 During its 2019 Outburst Observed with Insight-HXMT".Research in Astronomy and Astrophysics 22.11(2022). |
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