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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
高能物理研究所 [3]
采集方式
OAI收割 [3]
内容类型
期刊论文 [3]
发表日期
2019 [3]
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专题:高能物理研究所
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发表日期:2019
存缴方式:oaiharvest
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Insight-HXMT Observations of Swift J0243.6+6124 during Its 20172018 Outburst
期刊论文
OAI收割
The Astrophysical Journal, 2019, 卷号: 879
作者:
Zhang, Wei
;
Zhang, WanChang
;
Zhang, WenZhao
;
Zhang, Yi
;
Zhang, YiFei
  |  
收藏
  |  
浏览/下载:184/0
  |  
提交时间:2019/07/12
accretion
accretion disks
pulsars: individual: Swift J0243.6+6124
stars: distances
stars: magnetic field
X-rays: binaries
Astrophysics
- High Energy Astrophysical Phenomena
Super-Eddington Accretion onto the Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124
期刊论文
OAI收割
The Astrophysical Journal, 2019, 卷号: 873
作者:
Tao, Lian
;
Zhang, Yue
;
Feng, Hua
;
Zhang, Shuangnan
;
Bu, Qingcui
  |  
收藏
  |  
浏览/下载:46/0
  |  
提交时间:2019/07/12
accretion
accretion disks
magnetic fields
pulsars: individual:
Swift J0243.6+6124
stars: neutron
X-rays: binaries
Astrophysics -
High Energy Astrophysical Phenomena
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat
期刊论文
OAI收割
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:
HXMT
  |  
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  |  
浏览/下载:44/0
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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.