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浏览/检索结果: 共29条，第1-10条 帮助

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Accretion disk of a white hole 期刊论文  OAI收割
CHINESE PHYSICS C, 2025, 卷号: 49, 期号: 2, 页码: 11
作者:  Li LF(李丽仿);  Cao, Zhoujian;  Ling, Yi;  Wu, Xiaoning
  |  收藏  |  浏览/下载：4/0  |  提交时间：2025/02/24
Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling 期刊论文  OAI收割
UNIVERSE, 2022, 卷号: 8, 期号: 6, 页码: 13
作者:  Chang, Ning;  Liu, Xiang;  Xie, Fu-Guo;  Cui, Lang;  Shan, Hao
  |  收藏  |  浏览/下载：31/0  |  提交时间：2022/10/13
Influence of Irradiation-driven Winds on the Evolution of Intermediate-mass Black Hole X-ray Binaries 期刊论文  OAI收割
Astrophysical Journal, 2021, 卷号: 914, 期号: 2, 页码: 9109
作者:  Han, X. Q.;  Jiang, L.;  Chen, W. C.
  |  收藏  |  浏览/下载：25/0  |  提交时间：2022/06/30
The Jet-Disk Coupling of Seyfert Galaxies from a Complete Hard X-ray Sample 期刊论文  OAI收割
UNIVERSE, 2020, 卷号: 6, 期号: 5, 页码: 9
作者:  Liu, Xiang;  Chang, Ning;  Han, Zhenhua;  Wang, Xin
  |  收藏  |  浏览/下载：26/0  |  提交时间：2020/11/03
A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines 期刊论文  OAI收割
arXiv e-prints, 2018
作者:  Zhang, Chengmin;  Taani, Ali;  Chaty, Sylvain;  Karino, Shigeyuki;  Song, Liming
  |  收藏  |  浏览/下载：76/0  |  提交时间：2019/07/12
Astrophysics - High Energy Astrophysical Phenomena  Abstract: We have derived new physical quantities for several High-Mass X-ray Binaries (HMXBs) with supergiant (SG) companions through their cyclotron lines. The parameters are: the terminal velocity of the wind, the mass loss rate of the donor, the effective temperature and the magnetic fields. These parameters influence significantly the improvement of the model of accretion. In spite of the variety of their observational properties, the corresponding magnetic field is around B ~ 10^12 G. This result can be constrained by the effects on stellar evolution. In addition, we have performed a segmentation in the parameter space of donors intended for several SG-HMXB listed in our sample set. The parameter space can be categorized into five regimes depending on the possibility of disk formation associated with accretion from the stellar wind. This can give a quantitative clarification of the observed variability and the properties of these objects. We show that, when these systems come into the direct accretion region, systems with corresponding parameters can emit X-rays.  
State transitions triggered by inverse magnetic field: probably applied in high-mass X-ray binaries? 期刊论文  OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2016, 卷号: 16, 期号: 3
作者:  Li ShuangLiang;  Yan Zhen
  |  收藏  |  浏览/下载：7/0  |  提交时间：2021/12/06
Estimating Black Hole Spin of PG 1322+659 with Observed Optical and X-ray Continuum Spectrum 期刊论文  OAI收割
JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 2014, 卷号: 35, 期号: 3, 页码: 429-430
作者:  You, Bei;  Cao, Xinwu
收藏  |  浏览/下载：27/0  |  提交时间：2015/02/14
SUPERMASSIVE BLACK HOLES WITH HIGH ACCRETION RATES IN ACTIVE GALACTIC NUCLEI. II. THE MOST LUMINOUS STANDARD CANDLES IN THE UNIVERSE 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL, 2014, 卷号: 793, 期号: 2
作者:  SEAMBH collaboration
收藏  |  浏览/下载：33/0  |  提交时间：2015/12/02
Simulation of the emission lines radiated from cataclysmic variables 期刊论文  OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2013, 卷号: 13, 期号: 10, 页码: 1213-1218
作者:  He, Lin;  Lu, Guo-Liang;  Zhao, Yong-Heng;  Zhao Yongheng
收藏  |  浏览/下载：20/0  |  提交时间：2016/11/16
Determining the neutron star surface magnetic field strength of two Z sources 会议论文  OAI收割
IAU Symposium 290：Feeding Compact Objects: Accretion on All Scales, Beijing, China, 20 - 24 August 2012
作者:  Ding, Guoqiang;  Huang, Chunping;  Wang, Yanan
收藏  |  浏览/下载：26/0  |  提交时间：2016/07/28