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Compressed Magnetic Field in the Magnetically Regulated Global Collapsing Clump of G9.62+0.19 期刊论文
ASTROPHYSICAL JOURNAL LETTERS, 2018, 卷号: 869, 期号: 1, 页码: 6
作者:  Liu, Tie;  Kim, Kee-Tae;  Liu, Sheng-Yuan;  Juvela, Mika;  Zhang, Qizhou
收藏  |  浏览/下载:91/0  |  提交时间:2019/04/08
How Does the Stellar Wind Influence the Radio Morphology of a Supernova Remnant? 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 867, 期号: 1, 页码: 9
作者:  Zhang, M. F.;  Tian, W. W.;  Wu, D.
收藏  |  浏览/下载:0/0  |  提交时间:2020/03/10
Detection of 40-48 GHz dust continuum linear polarization towards the Class 0 young stellar object IRAS 16293-2422 期刊论文
ASTRONOMY & ASTROPHYSICS, 2018, 卷号: 617, 页码: 15
作者:  Liu, Hauyu Baobab;  Hasegawa, Yasuhiro;  Ching, Tao-Chung;  Lai, Shih-Ping;  Hirano, Naomi
收藏  |  浏览/下载:18/0  |  提交时间:2020/03/10
The spin of the second-born black hole in coalescing binary black holes 期刊论文
ASTRONOMY & ASTROPHYSICS, 2018, 卷号: 616
作者:  Qin, Y.;  Fragos, T.;  Meynet, G.;  Andrews, J.;  Sorensen, M.
收藏  |  浏览/下载:24/0  |  提交时间:2018/09/10
The straight and isolated G350.54+0.69 filament: density profile and star formation content 期刊论文
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 卷号: 478, 期号: 2, 页码: 2119-2131
作者:  Liu, Hong-Li;  Stutz, Amelia;  Yuan, Jing-Hua
收藏  |  浏览/下载:65/0  |  提交时间:2020/03/10
Calvera: A Low-mass Strangeon Star Torqued by Debris Disk? 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 854, 期号: 2, 页码: 9
作者:  Li, Yunyang;  Wang, Weiyang;  Ge, Mingyu;  Liu, Xiongwei;  Tong, Hao
收藏  |  浏览/下载:1/0  |  提交时间:2020/03/11
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.  
Calvera: A Low-mass Strangeon Star Torqued by Debris Disk? 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 854, 期号: 2, 页码: 165
作者:  Ge MY(葛明玉);  Wang, WY;  Li, YY;  Xu, RX;  Tong, H
收藏  |  浏览/下载:21/0  |  提交时间:2019/09/24
Star-Disk Interactions in Multiband Photometric Monitoring of the Classical T Tauri Star GI Tau 期刊论文
ASTROPHYSICAL JOURNAL, 2018, 卷号: 852, 期号: 1, 页码: 56
作者:  Michel, Raul;  Chiang, Po-Shih;  Fu, Jianning;  Jose, Jessy;  Herczeg, Gregory J.
收藏  |  浏览/下载:58/0  |  提交时间:2018/08/29


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