中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
机构
采集方式
内容类型
发表日期
学科主题
筛选

浏览/检索结果: 共9条,第1-9条 帮助

条数/页: 排序方式:
The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2024, 卷号: 67, 期号: 1
作者:  
Xiang, Danfeng;  Mo, Jun;  Wang, Lingzhi;  Wang, Xiaofeng;  Zhang JJ(张居甲)
  |  收藏  |  浏览/下载:18/0  |  提交时间:2024/03/29
Adiabatic Mass Loss in Binary Stars. III. From the Base of the Red Giant Branch to the Tip of the Asymptotic Giant Branch 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL, 2020, 卷号: 899, 期号: 2, 页码: 15
作者:  
Ge HW(葛宏伟);  Webbink, Ronald F.;  Chen XF(陈雪飞);  Han ZW(韩占文)
  |  收藏  |  浏览/下载:34/0  |  提交时间:2020/10/26
The Thermal Equilibrium Mass-loss Model and Its Applications in Binary Evolution 期刊论文  OAI收割
The Astrophysical Journal Supplement Series, 2020, 卷号: 249, 期号: 1, 页码: 1-18
作者:  
Ge HW(葛宏伟);  Ronald F Webbink;  Han ZW(韩占文)
  |  收藏  |  浏览/下载:50/0  |  提交时间:2020/07/27
Mind the Gap: The Location of the Lower Edge of the Pair-instability Supernova Black Hole Mass Gap 期刊论文  OAI收割
The Astrophysical Journal, 2019, 卷号: 887, 期号: 1
作者:  
Farmer,R.;  Renzo,M.;  de Mink,S. E.;  Marchant,P.;  Justham,S.
  |  收藏  |  浏览/下载:101/0  |  提交时间:2020/03/10
Observatory science with eXTP 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2019, 卷号: 62, 期号: 2, 页码: 42
作者:  
in't Zand, Jean J. M.;  Bozzo, Enrico;  Qu, JinLu;  Li, Xiang-Dong;  Amati, Lorenzo
  |  收藏  |  浏览/下载:161/0  |  提交时间:2019/04/08
Observatory science with eXTP 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2019, 卷号: 62, 期号: 2
作者:  
in't Zand, Jean J. M.;  Bozzo, Enrico;  Qu, JinLu;  Li, Xiang-Dong;  Amati, Lorenzo
  |  收藏  |  浏览/下载:146/0  |  提交时间:2019/05/23
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:75/0  |  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.  
The effects of solar Reimers eta on the final destinies of Venus, the Earth, and Mars 期刊论文  OAI收割
Astrophysics and Space Science, 2016, 卷号: 361, 期号: 4, 页码: 122
作者:  
Guo, Jianpo;  Lin, Ling;  Bai, Chunyan;  Liu, Jinzhong
  |  收藏  |  浏览/下载:28/0  |  提交时间:2019/12/09
The initial-final mass relation of stars 期刊论文  OAI收割
CHINESE ASTRONOMY AND ASTROPHYSICS, 1998, 卷号: 22, 期号: 1, 页码: 41-48
作者:  
Han ZW(韩占文);  Han, ZW
收藏  |  浏览/下载:16/0  |  提交时间:2016/04/05