×
验证码:
换一张
忘记密码?
记住我
CORC
首页
科研机构
检索
知识图谱
申请加入
托管服务
登录
注册
在结果中检索
科研机构
高能物理研究所 [4]
国家天文台 [3]
内容类型
期刊论文 [7]
发表日期
2018 [7]
×
知识图谱
CORC
开始提交
已提交作品
待认领作品
已认领作品
未提交全文
收藏管理
QQ客服
官方微博
反馈留言
浏览/检索结果:
共7条,第1-7条
帮助
限定条件
发表日期:2018
内容类型:期刊论文
已选(
0
)
清除
条数/页:
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
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
Laboratory study of astrophysical collisionless shock at SG-II laser facility
期刊论文
HIGH POWER LASER SCIENCE AND ENGINEERING, 2018, 卷号: 6, 页码: 8
作者:
Yuan, Dawei
;
Wei, Huigang
;
Liang, Guiyun
;
Wang, Feilu
;
Li, Yutong
收藏
  |  
浏览/下载:16/0
  |  
提交时间:2020/03/10
collisionless shock
electromagnetic field
high power lasers
laboratory astrophysics
Massive Outflows Associated with ATLASGAL Clumps
期刊论文
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2018, 卷号: 235, 期号: 1, 页码: 20
作者:
Yang, A. Y.
;
Thompson, M. A.
;
Urquhart, J. S.
;
Tian, W. W.
收藏
  |  
浏览/下载:0/0
  |  
提交时间:2020/03/11
ISM: jets and outflows
ISM: molecules
stars: early-type
stars: formation
stars: massive
submillimeter: ISM
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.
Constraining axion-like-particles with hard X-ray emission from magnetars
期刊论文
Journal of High Energy Physics, 2018, 卷号: 2018
作者:
Sinha, Kuver
;
Fortin, Jean-François
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2019/07/12
Cosmology of Theories beyond the SM
Beyond Standard Model
CP
violation
High Energy Physics - Phenomenology
Astrophysics - High
Energy Astrophysical Phenomena
A low-latency pipeline for GRB light curve and spectrum using Fermi/GBM near real-time data
期刊论文
Research in Astronomy and Astrophysics, 2018, 卷号: 18
作者:
Shao, Jian-Xiong
;
Li, Han-Cheng
;
Bu, Qing-Cui
;
Feng, Min-Zi
;
Li, Zheng-Heng
收藏
  |  
浏览/下载:46/0
  |  
提交时间:2019/07/12
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
The GeV emission of PSR B1259-63 during its last three periastron passages observed by Fermi-LAT
期刊论文
Research in Astronomy and Astrophysics, 2018, 卷号: 18
作者:
Zhang, Shu
;
Chen, Yu-Peng
;
Kong, Ling-Da
;
Ji, Long
;
Liu, Cong-Zhan
收藏
  |  
浏览/下载:19/0
  |  
提交时间:2019/07/12
Astrophysics - High Energy Astrophysical Phenomena
laboratorystudyofastrophysicalcollisionlessshockatsgiilaserfacility
期刊论文
highpowerlaserscienceandengineering, 2018, 卷号: 6, 期号: 3
作者:
Yuan Dawei
;
Wei Huigang
;
Liang Guiyun
;
Wang Feilu
;
Li Yutong
收藏
  |  
浏览/下载:3/0
  |  
提交时间:2020/03/11
©版权所有 ©2017 CSpace - Powered by
CSpace