CORC

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CORC

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Insight-HXMT Observations of a Possible Fast Transition from the Jet- to Wind-dominated State during a Huge Flare of GRS 1915+105 期刊论文
The Astrophysical Journal, 2021, 卷号: 906, 页码: L2
作者:  Kong, L. D.;  Zhang, S.;  Chen, Y. P.;  Zhang, S. N.;  Ji, L.
收藏  |  浏览/下载：14/0  |  提交时间：2021/11/18
IPN Triangulation of GRB 200120A GCN
2020
作者:  Hurley, K;  Mitrofanov, I. G;  Golovin, D. V;  Kozyrev, A. S;  Litvak, M. L
收藏  |  浏览/下载：28/0  |  提交时间：2020/05/20
IPN triangulation of GRB 200111A GCN
2020
作者:  Hurley, K;  Mitrofanov, I. G;  Golovin, D. V;  Kozyrev, A. S;  Litvak, M. L
收藏  |  浏览/下载：24/0  |  提交时间：2020/05/20
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition 期刊论文
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:  HXMT
收藏  |  浏览/下载：15/0  |  提交时间：2022/02/08
First performance test of a 30 mm iron-based superconductor single pancake coil under a 24 t background field 期刊论文
Superconductor science and technology, 2019, 卷号: 32, 期号: 4
作者:  Wang,Dongliang;  Zhang,Zhan;  Zhang,Xianping;  Jiang,Donghui;  Dong,Chiheng
收藏  |  浏览/下载：73/0  |  提交时间：2019/04/23
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：67/0  |  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.  
Explanation of the Knee-like Feature in the DAMPE Cosmic e(-) + e(+) Energy Spectrum 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 854, 期号: 1, 页码: 57
作者:  Yin, PF;  Fang K(方堃);  Bi XJ(毕效军);  Yin PF(殷鹏飞);  Fang, K
收藏  |  浏览/下载：33/0  |  提交时间：2019/09/24
Perspective on the Cosmic-ray Electron Spectrum above TeV 期刊论文
ASTROPHYSICAL JOURNAL, 2017, 卷号: 836, 期号: 2, 页码: 172
作者:  Wang, BB;  Yin, PF;  Lin, SJ;  Bi, XJ;  Fang, K
收藏  |  浏览/下载：20/0  |  提交时间：2019/08/27
WIND BRAKING OF MAGNETARS 期刊论文
ASTROPHYSICAL JOURNAL, 2013, 卷号: 768, 期号: 2, 页码: 144
作者:  Tong H(仝号);  Tong, H;  Xu, 宋黎明;  RX;  Song, LM
收藏  |  浏览/下载：15/0  |  提交时间：2016/04/08
风场环境下平流层飞艇运动建模 期刊论文
系统科学与数学, 2013, 期号: 6, 页码: 685-694
作者:  苗景刚;  王帆;  周江华;  姜鲁华
收藏  |  浏览/下载：12/0  |  提交时间：2015/12/15

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