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CAS IR Grid
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国家天文台 [39]
高能物理研究所 [29]
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Science Goals of the Earth 2.0 Space Mission
会议论文
OAI收割
Montreal, CANADA, JUL 17-22, 2022
作者:
Zhang, Hui
;
Ge, Jian
;
Deng, Hongping
;
Yao, Xinyu
;
Zhu, Jiapeng
  |  
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2023/06/28
ET
Earth 2.0
terrestrial planet
habitable planet
free-floating
planet
time-domain
black-hole
binary stars
Wavelet analysis of the transient QPOs in MAXI J1535-571 with Insight-HXMT
期刊论文
OAI收割
Monthly Notices of the Royal Astronomical Society, 2022, 卷号: 517, 期号: 1, 页码: 182
作者:
Chen, X.
;
Wang, W.
;
Tian, P. F.
;
Zhang, P.
;
Liu, Q.
  |  
收藏
  |  
浏览/下载:10/0
  |  
提交时间:2023/11/10
black hole physics
Stars: individual: MAXI J1535-571
X-rays: binaries
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - Solar and Stellar Astrophysics
Re-estimating the Spin Parameter of the Black Hole in Cygnus X-1
期刊论文
OAI收割
The Astrophysical Journal, 2021, 卷号: 908, 期号: 2
作者:
Zhao,Xueshan
;
Gou,Lijun
;
Dong,Yanting
;
Zheng,Xueying
;
Steiner,James F.
  |  
收藏
  |  
浏览/下载:29/0
  |  
提交时间:2021/12/06
X-ray binary stars
Black hole physics
High energy astrophysics
Synchronous X-ray/Optical QPOs from the Black Hole LMXB MAXI J1820+070
期刊论文
OAI收割
Monthly Notices of the Royal Astronomical Society, 2021
作者:
HXMT
  |  
收藏
  |  
浏览/下载:53/0
  |  
提交时间:2022/02/08
black hole physics
Low Mass X-ray Binaries
accretion
accretion
discs
stars: individual (MAXI J1820+070)
Astrophysics - High Energy
Astrophysical Phenomena
Abstract: We present high-speed optical photometry from SAAO and SALT on the black hole LMXB MAXI J1820+070 (ASSASN-18ey), some of it simultaneous with NICER, Swift and Insight-HXMT X-ray coverage. We detect optical Quasi-Periodic Oscillations (QPOs) that move to higher frequencies as the outburst progresses, tracking both the frequency and evolution of similar X-ray QPOs previously reported. Correlated X-ray/optical data reveal a complex pattern of lags, including an anti-correlation and a sub-second lag that evolve over the first few weeks of outburst. They also show correlated components separated by a lag equal to the QPO period roughly centered on zero lag, implying that the inter-band variability is strongly and consistently affected by these QPOs at a constant phase lag of roughly ±Ю The synchronisation of X-ray and optical QPOs indicates that they must be produced in regions physically very close to each other
we thus propose that they can be explained by a precessing jet model, based on analogies with V404 Cyg and MAXI J1348-630.
Phase-dependent Study of Near-infrared Disk Emission Lines in LB-1
期刊论文
OAI收割
The Astrophysical Journal, 2020, 卷号: 900, 期号: 1
作者:
Liu,Jifeng
;
Zheng,Zheng
;
Soria,Roberto
;
Aceituno,Jesus
;
Zhang,Haotong
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收藏
  |  
浏览/下载:34/0
  |  
提交时间:2021/12/06
Black holes
black hole physics
Stellar evolution
Be stars
Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes
期刊论文
OAI收割
ASTRONOMY & ASTROPHYSICS, 2020, 卷号: 636, 页码: 40
作者:
Belczynski, K.
;
Klencki, J.
;
Fields, C. E.
;
Olejak, A.
;
Berti, E.
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收藏
  |  
浏览/下载:28/0
  |  
提交时间:2021/12/06
stars: massive
black hole physics
gravitational waves
Radio/X-Ray Correlation in the Mini-outbursts of Black Hole X-Ray Transient GRS 1739-278
期刊论文
OAI收割
ASTROPHYSICAL JOURNAL, 2020, 卷号: 891, 期号: 1, 页码: 9
作者:
Xie, Fu-Guo
;
Yan, Zhen
;
Wu, Zhongzu
  |  
收藏
  |  
浏览/下载:13/0
  |  
提交时间:2021/09/26
Stellar accretion disks
black hole physics
X-ray binary stars
Low-mass x-ray binary stars
Luminous Red Novae: population models and future prospects
期刊论文
OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 卷号: 492, 期号: 3, 页码: 3229-3240
作者:
Howitt, George
;
Stevenson, Simon
;
Vigna-Gomez, Alejandro
;
Justham, Stephen
;
Ivanova, Natasha
  |  
收藏
  |  
浏览/下载:92/0
  |  
提交时间:2021/09/26
black hole physics
gravitational waves
stars: evolution
The Formation of a 70 M⊙ Black Hole at High Metallicity
期刊论文
OAI收割
The Astrophysical Journal, 2020, 卷号: 890, 期号: 2
作者:
Belczynski,K.
;
Hirschi,R.
;
Kaiser,E. A.
;
Liu,Jifeng
;
Casares,J.
  |  
收藏
  |  
浏览/下载:64/0
  |  
提交时间:2021/09/26
Black hole physics
Classical black holes
Binary stars
Jets in the soft state in Cyg X-3 caused by advection of the donor magnetic field and unification with low-mass X-ray binaries
期刊论文
OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 卷号: 492, 期号: 1, 页码: 223-231
作者:
Cao, Xinwu
;
Zdziarski, Andrzej A.
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收藏
  |  
浏览/下载:40/0
  |  
提交时间:2021/09/26
accretion, accretion discs
black hole physics
magnetic fields
stars: individual: Cyg X-3
X-rays: binaries