INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535?571: Timing Analysis
文献类型:期刊论文
作者 | Fu, M. X; Ge, M. Y; Gu, Y. D; Guan, J; Gungor, C; Guo, C. C; Han, D. W; Hu, W; Huo, J; Ji, J. F |
刊名 | The Astrophysical Journal |
出版日期 | 2018 |
卷号 | 866期号:2页码:122 |
关键词 | black hole physics stars: individual (MAXI J1535-571) X-rays: binaries |
DOI | 10.3847/1538-4357/aade4c |
英文摘要 | 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. |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000456435200005 |
源URL | [http://ir.ihep.ac.cn/handle/311005/282271] |
专题 | 硬X射线调制望远镜卫星 |
推荐引用方式 GB/T 7714 | Fu, M. X,Ge, M. Y,Gu, Y. D,et al. INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535?571: Timing Analysis[J]. The Astrophysical Journal,2018,866(2):122. |
APA | Fu, M. X.,Ge, M. Y.,Gu, Y. D.,Guan, J.,Gungor, C.,...&Collaboration, The Insight-HXMT .(2018).INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535?571: Timing Analysis.The Astrophysical Journal,866(2),122. |
MLA | Fu, M. X,et al."INSIGHT-HXMT Observations of the New Black Hole Candidate MAXI J1535?571: Timing Analysis".The Astrophysical Journal 866.2(2018):122. |
入库方式: OAI收割
来源:高能物理研究所
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