| INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535-571: Timing Analysis | |
Huang, Y.1,2; Qu, J. L.1; Zhang, S. N.1,2; Bu, Q. C.1; Chen, Y. P.1; Tao, L.1; Zhang, S.1; Lu, F. J.1; Li, T. P.1,2,3; Song, L. M.1; Xu, Y. P.1; Cao, X. L.1; Chen, Y.1; Liu, C. Z.1; Chang, H. -K.4,5; Yu, W. F.6; Weng, S. S.7; Hou X(侯贤)8,9,10 ; Kong, A. K. H.4; Xie, F. G.6; Zhang GB(张国宝)8,9,10; Zhou, J. F.3; Chang, Z.1; Chen, G.1; Chen, L.11; Chen, T. X.1; Chen, Y. B.3; Cui, W.1,3; Cui, W. W.1; Deng, J. K.3; Dong, Y. W.1; Du, Y. Y.1; Fu, M. X.3; Gao, G. H.1,2; Gao, H.1,2; Gao, M.1; Ge, M. Y.1; Gu, Y. D.1; Guan, J.1; Gungor, C.1; Guo, C. C.1,2; Han, D. W.1; Hu, W.1; Huo, J.1; Ji, J. F.2; Jia, S. M.1; Jiang, L. H.1; Jiang, W. C.1; Jin, J.1; Jin, Y. J.12; Li, B.1; Li, C. K.1; Li, G.1; Li, M. S.1; Li, W.1; Li, X.1; Li, X. B.1; Li, X. F.1; Li, Y. G.1; Li, Z. J.1,2; Li, Z. W.1; Liang, X. H.1; Liao, J. Y.1; Liu, G. Q.3; Liu, H. W.1; Liu, S. Z.1; Liu, X. J.1; Liu, Y.1; Liu, Y. N.12; Lu, B.1; Lu, X. F.1; Luo, T.1; Ma, X.1; Meng, B.1; Nang, Y.1,2; Nie, J. Y.1; Ou, G.1; Sai, N.1,2; Shang, R. C.3; Sun, L.1; Tan, Y.1; Tao, W.1; Tuo, Y. L.1,2; Wang, G. F.1; Wang, H. Y.1; Wang, J.1; Wang, W. S.1; Wang, Y. S.1; Wen, X. Y.1; Wu, B. B.1; Wu, M.1; Xiao, G. C.1,2; Xiong, S. L.1; Xu, H.1; Yan, L. L.1,2; Yang, J. W.1; Yang, S.1; Yang, Y. J.1; Zhang, A. M.1; Zhang, C. L.1; Zhang, C. M.1; Zhang, F.1; Zhang, H. M.1; Zhang, J.1; Zhang, Q.1; Zhang, T.1; Zhang, W.1,2; Zhang, W. C.1; Zhang, W. Z.12; Zhang, Y.1; Zhang, Y.1,2; Zhang, Y. F.1; Zhang, Y. J.1; Zhang, Z.3; Zhang, Z.11; Zhang, Z. L.1; Zhao, H. S.1; Zhao, J. L.1; Zhao, X. F.1,2; Zheng, S. J.1; Zhu, Y.1; Zhu, Y. X.1; Zou, C. L.1
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| 发表期刊 | ASTROPHYSICAL JOURNAL
 |
| 2018-10-20 | |
| 卷号 | 866期号:2页码:10 |
| DOI | 10.3847/1538-4357/aade4c |
| 产权排序 | 第8完成单位 |
| 收录类别 | SCI |
| 关键词 | black hole physics stars: individual (MAXI J1535-571) X-rays: binaries |
| 摘要 | We present X-ray timing results of the new black hole candidate MAXI J1535-571 during its 2017 outburst from Hard X-ray Modulation Telescope (Insight-HXMT) observations taken from 2017 September 6 to 23. Following the definitions given by Belloni, we find that the source exhibits transitions from the low/hard state to the hard intermediate state, and eventually to the soft intermediate state. Quasi-periodic oscillations (QPOs) are found in the intermediate states, which suggest different types of QPOs. With the large effective area of Insight-HXMT at high energies, we are able to present the energy dependence of the QPO amplitude and centroid frequency up to 100 keV, which has rarely been explored by previous satellites. We also find that the phase lag at the type-C QPOs centroid frequency is negative (soft lag) and strongly correlated with the centroid frequency. Assuming a geometrical origin of type-C QPOs, the source is consistent with being a high-inclination system. |
| 资助项目 | China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; National Program on Key Research and Development Project[2016YFA0400800] ; National Natural Science Foundation of China[U1838108] ; National Natural Science Foundation of China[11733009] ; National Natural Science Foundation of China[11673023] ; National Natural Science Foundation of China[U1838110] ; National Natural Science Foundation of China[U1838113] ; National Natural Science Foundation of China[U1838111] ; National Natural Science Foundation of China[U1838115] ; National Natural Science Foundation of China[U1838201] ; CAS Pioneer Hundred Talent Program[Y8291130K2] ; Scientific and technological innovation project of IHEP[Y7515570U1] |
| 项目资助者 | China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; National Program on Key Research and Development Project[2016YFA0400800] ; National Natural Science Foundation of China[U1838108, 11733009, 11673023, U1838110, U1838113, U1838111, U1838115, U1838201] ; CAS Pioneer Hundred Talent Program[Y8291130K2] ; Scientific and technological innovation project of IHEP[Y7515570U1] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 |
| 文章类型 | Article |
| 出版者 | IOP PUBLISHING LTD |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000456435200005 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | QUASI-PERIODIC OSCILLATIONS ; X-RAY-PROPERTIES ; ENERGY-DEPENDENCE ; PHASE-LAG ; GX 339-4 ; CENTROID FREQUENCY ; GRS 1915+105 ; VARIABILITY ; MODULATION ; EVOLUTION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/19198 |
| 专题 | 高能天体物理研究组 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Huang, Y. |
| 作者单位 | 1.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People's Republic of China 2.University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, People's Republic of China 3.Department of Physics, Tsinghua University, Beijing 100084, People's Republic of China 4.Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan 5.Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan 6.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People's Republic of China 7.Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing 210023, People's Republic of China 8.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China 9.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China 10.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, People's Republic of China 11.Department of Astronomy, Beijing Normal University, Beijing 100088, People's Republic of China 12.Department of Engineering Physics, Tsinghua University, Beijing 100084, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Huang, Y.,Qu, J. L.,Zhang, S. N.,et al. INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535-571: Timing Analysis[J]. ASTROPHYSICAL JOURNAL,2018,866(2):10. |
| APA | Huang, Y..,Qu, J. L..,Zhang, S. N..,Bu, Q. C..,Chen, Y. P..,...&Zou, C. L..(2018).INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535-571: Timing Analysis.ASTROPHYSICAL JOURNAL,866(2),10. |
| MLA | Huang, Y.,et al."INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535-571: Timing Analysis".ASTROPHYSICAL JOURNAL 866.2(2018):10. |
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| INSIGHT-HXMT Observa（1482KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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