中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
DOI10.3847/1538-4357/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
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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.

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