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浏览/检索结果: 共5条，第1-5条 帮助 已选(0)清除 条数/页：5101520253035404550556065707580859095100   排序方式：请选择作者升序作者降序题名升序题名降序发表日期升序发表日期降序提交时间升序提交时间降序 Black holes, gravitational waves and fundamental physics: a roadmap 期刊论文 CLASSICAL AND QUANTUM GRAVITY, 2019, 卷号: 36, 期号: 14, 页码: 178 作者:  Barack, Leor;  Cardoso, Vitor;  Nissanke, Samaya;  Sotiriou, Thomas P.;  Askar, Abbas 收藏  |  浏览/下载：170/0  |  提交时间：2019/09/26 gravitational waves  gravitational-wave astronomy  source modelling  black holes  fundamental physics  birth and evolution of black holes   Black holes, gravitational waves and fundamental physics: a roadmap 期刊论文 CLASSICAL AND QUANTUM GRAVITY, 2019, 卷号: 36, 期号: 14, 页码: 178 作者:  Barack, Leor;  Cardoso, Vitor;  Nissanke, Samaya;  Sotiriou, Thomas P.;  Askar, Abbas 收藏  |  浏览/下载：109/0  |  提交时间：2019/10/28 gravitational waves  gravitational-wave astronomy  source modelling  black holes  fundamental physics  birth and evolution of black holes   A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines 期刊论文 arXiv e-prints, 2018 作者:  Zhang, Chengmin;  Taani, Ali;  Chaty, Sylvain;  Karino, Shigeyuki;  Song, Liming 收藏  |  浏览/下载：66/0  |  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.   MULTI-WAVELENGTH STUDY OF THE Be/X-RAY BINARY MXB 0656-072 期刊论文 ASTROPHYSICAL JOURNAL, 2012, 卷号: 753, 期号: 1, 页码: 73(11pp) 作者:  Yan, Jingzhi;  Heras, Juan Antonio Zurita;  Chaty, Sylvain;  Li, Hui;  Liu, Qingzhong 收藏  |  浏览/下载：14/0  |  提交时间：2013/01/31 stars: emission-line, Be  stars: individual (MXB 0656-072)  stars: neutron  X-rays: binaries   MODELING THE HARD STATES OF THREE BLACK HOLE CANDIDATES 期刊论文 ASTROPHYSICAL JOURNAL, 2010, 卷号: 717, 期号: 2, 页码: 929-936 作者:  Zhang, Hui;  Yuan, Feng;  Chaty, Sylvain 收藏  |  浏览/下载：14/0  |  提交时间：2011/06/29 accretion  accretion disks  black hole physics  ISM: jets and outflows  stars: individual (SWIFT J1753.5-0127  GRO J1655-40  XTE J1720-319)