机构

• 国家天文台 [5]
• 紫金山天文台 [3]
• 云南天文台 [2]
• 上海天文台 [1]
• 高能物理研究所 [1]

采集方式

• OAI收割 [12]

内容类型

• 期刊论文 [12]

发表日期

• 2021 [2]
• 2020 [4]
• 2019 [2]
• 2018 [1]
• 2006 [1]
• 2002 [2]
• 更多

学科主题

• Astronomy ... [1]
• 天文学 [1]
• 天文学::恒星与银河... [1]
• 天文学::恒星与银河... [1]
• 天文学::恒星与银河... [1]

筛选

浏览/检索结果: 共12条，第1-10条 帮助 条数/页： 5101520253035404550556065707580859095100 排序方式： 请选择题名升序题名降序提交时间升序提交时间降序作者升序作者降序发表日期升序发表日期降序 The Old Moving Groups in the Field of Taurus 期刊论文  OAI收割 The Astrophysical Journal Supplement Series, 2021, 卷号: 254, 期号: 1 作者:  Liu,Jiaming;  Fang,Min;  Tian,Hao;  Liu,Chao;  Yang,Chengqun   |  收藏  |  浏览/下载：42/0  |  提交时间：2021/12/06 Pre-main sequence stars  Young stellar objects  Stellar accretion  Accretion  Stellar accretion disks  Star clusters  Stellar associations  Star formation  Star-forming regions   What Produces Dust Polarization in the HH 212 Protostellar Disk at 878 μm: Dust Self-scattering or Dichroic Extinction? 期刊论文  OAI收割 The Astrophysical Journal, 2021, 卷号: 910, 期号: 1 作者:  Lee,Chin-Fei;  Li,Zhi-Yun;  Yang,Haifeng;  Daniel Lin,Zhe-Yu;  Ching,Tao-Chung   |  收藏  |  浏览/下载：23/0  |  提交时间：2021/12/06 Star formation  Accretion  Young stellar objects  Polarimetry  Magnetic fields   Long-term Period Changes and Brightness Variations for the Deeply Eclipsing Cataclysmic Variable SW Sex 期刊论文  OAI收割 ASTROPHYSICAL JOURNAL, 2020, 卷号: 901, 期号: 2, 页码: 8 作者:  Fang XH(方小慧);  Qian SB(钱声帮);  Han ZT(韩忠涛);  Wang QS(王琪善)   |  收藏  |  浏览/下载：36/0  |  提交时间：2020/11/30 Nova-like variable stars  Stellar evolution  Stellar winds  Stellar accretion disks  CCD photometry   Two Complete Spectral Transitions of Swift J0243.6+6124 Observed by Insight-HXMT 期刊论文  OAI收割 The Astrophysical Journal, 2020, 卷号: 902, 期号: 1 作者:  Kong,L. D.;  Zhang,S.;  Chen,Y. P.;  Zhang,S. N.;  Ji,L.   |  收藏  |  浏览/下载：22/0  |  提交时间：2021/12/06 Accretion  Stellar accretion disks  Binary pulsars  Magnetic fields  Neutron stars  X-ray binary stars  X-ray astronomy   Discovery of the Black Hole X-Ray Binary Transient MAXI J1348–630 期刊论文  OAI收割 The Astrophysical Journal Letters, 2020, 卷号: 899, 期号: 1 作者:  Tominaga,Mayu;  Nakahira,Satoshi;  Shidatsu,Megumi;  Oeda,Motoki;  Ebisawa,Ken   |  收藏  |  浏览/下载：21/0  |  提交时间：2021/12/06 Black holes  Compact objects  High energy astrophysics  X-ray novae  Stellar accretion disks   Radio/X-Ray Correlation in the Mini-outbursts of Black Hole X-Ray Transient GRS 1739-278 期刊论文  OAI收割 ASTROPHYSICAL JOURNAL, 2020, 卷号: 891, 期号: 1, 页码: 9 作者:  Xie, Fu-Guo;  Yan, Zhen;  Wu, Zhongzu   |  收藏  |  浏览/下载：13/0  |  提交时间：2021/09/26 Stellar accretion disks  black hole physics  X-ray binary stars  Low-mass x-ray binary stars   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 space research instruments  nuclear astrophysics  flare stars  accretion and accretion disks  mass loss and stellar winds  cataclysmic binaries  X-ray binaries  supernova remnants  active galactic nuclei  X-ray bursts  gamma-ray bursts  gravitational waves   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 Space Research Instruments  Nuclear Astrophysics  Flare Stars  Accretion And Accretion Disks  Mass Loss And Stellar Winds  Cataclysmic Binaries  X-ray Binaries  Supernova Remnants  Active Galactic Nuclei  X-ray Bursts  Gamma-ray Bursts  Gravitational Waves   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.   Population synthesis for symbiotic stars with white dwarf accretors 期刊论文  OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 卷号: 372, 期号: 3, 页码: 1389-1406 作者:  Lv GL(吕国梁);  Yungelson, L;  Han ZW(韩占文) 收藏  |  浏览/下载：16/0  |  提交时间：2016/04/05 accretion, accretion discs  binaries : symbiotic  stars : evolution  white dwarfs  Galaxy : stellar content