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科研机构
高能物理研究所 [78]
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期刊论文 [77]
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2021 [6]
2020 [3]
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Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT
期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 94
作者:
Ma, Xiang
;
Tao, Lian
;
Zhang, Shuang-Nan
;
Zhang, Liang
;
Bu, Qing-Cui
收藏
  |  
浏览/下载:66/0
  |  
提交时间:2021/11/18
A Variable Ionized Disk Wind in the Black Hole Candidate EXO 1846-031
期刊论文
The Astrophysical Journal, 2021, 卷号: 906, 页码: 11
作者:
Wang, Yanan
;
Ji, Long
;
García, Javier A.
;
Dauser, Thomas
;
Méndez, Mariano
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  |  
浏览/下载:29/0
  |  
提交时间:2021/11/18
Detection of a Low-frequency Quasi-periodic Oscillation in the Soft State of Cygnus X-1 with Insight-HXMT
期刊论文
The Astrophysical Journal, 2021, 卷号: 919, 页码: 46
作者:
Yan, Zhen
;
Rapisarda, Stefano
;
Yu, Wenfei
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  |  
浏览/下载:8/0
  |  
提交时间:2021/11/18
Time-lag Between Disk and Corona Radiation Leads to Hysteresis Effect Observed in Black hole X-Ray Binary MAXI J1348-630
期刊论文
The Astrophysical Journal, 2021, 卷号: 915, 页码: L15
作者:
Weng, Shan-Shan
;
Cai, Zhen-Yi
;
Zhang, Shuang-Nan
;
Zhang, Wei
;
Chen, Yu-Peng
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  |  
浏览/下载:11/0
  |  
提交时间:2021/11/18
Physical origin of the non-physical spin evolution of MAXI J1820 + 070
期刊论文
Monthly Notices of the Royal Astronomical Society, 2021, 卷号: 504, 页码: 2168
作者:
Guan, J.
;
Tao, L.
;
Qu, J. L.
;
Zhang, S. N.
;
Zhang, W.
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浏览/下载:56/0
  |  
提交时间:2021/11/18
accretion
accretion discs
black hole physics
stars: individual
(MAXI J1820 + 070)
X-rays: binaries
Astrophysics - High Energy
Astrophysical Phenomena
83C57
Synchronous X-ray/Optical QPOs from the Black Hole LMXB MAXI J1820+070
期刊论文
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2021, 2021
作者:
HXMT
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浏览/下载:45/0
  |  
提交时间:2022/02/08
black hole physics
Low Mass X-ray Binaries
accretion
accretion
discs
stars: individual (MAXI J1820+070)
black hole physics
Low Mass X-ray Binaries
accretion
accretion
discs
stars: individual (MAXI J1820+070)
Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT
期刊论文
Nature Astronomy, 2020
作者:
Xiang Ma
;
Lian Tao
;
Shuang-Nan Zhang
;
Liang Zhang
;
Qing-Cui Bu
;
Ming-Yu Ge
;
Yu-Peng Chen
;
Jin-Lu Qu
;
Shu Zhang
;
Fang-Jun Lu
;
Li-Ming Song
;
Yi-Jung Yang
;
Feng Yuan
;
Ce Cai
;
Xue-Lei Cao
;
Zhi Chang
;
Gang Chen
;
Li Chen
;
Tian-Xiang Chen
;
Yi-Bao Chen
;
Yong Chen
;
Wei Cui
;
Wei-Wei Cui
收藏
  |  
浏览/下载:12/0
  |  
提交时间:2020/09/23
Joint analysis of energy and RMS spectra from MAXI J1535-571 with Insight-HXMT
期刊论文
Journal of High Energy Astrophysics, 2020, 卷号: 25, 页码: 29-38
作者:
The Insight-HXMT Collaboration
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  |  
浏览/下载:29/0
  |  
提交时间:2020/03/27
Starts: individual (MAXI J1535-571)
X-rays: binaries
Black hole physics
An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242
期刊论文
Astronomy and Astrophysics, 2020, 卷号: 641, 页码: A101
作者:
HXMT
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2022/02/08
accretion
accretion disks
black hole physics
X-rays: binaries
time
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat
期刊论文
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:
HXMT
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  |  
浏览/下载:41/0
  |  
提交时间:2022/02/08
Accretion
accretion disks
Black hole physics
X-rays: binaries:
Swift J1658.2-4242
Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.
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