咨询与建议

限定检索结果

文献类型

  • 1,000 篇 期刊文献
  • 12 篇 会议

馆藏范围

  • 1,012 篇 电子文献
  • 0 种 纸本馆藏

日期分布

学科分类号

  • 962 篇 理学
    • 630 篇 地球物理学
    • 357 篇 物理学
    • 250 篇 天文学
    • 118 篇 数学
    • 97 篇 化学
    • 63 篇 统计学(可授理学、...
    • 26 篇 地质学
    • 20 篇 大气科学
    • 18 篇 系统科学
  • 513 篇 工学
    • 151 篇 电子科学与技术(可...
    • 117 篇 电气工程
    • 104 篇 仪器科学与技术
    • 100 篇 动力工程及工程热...
    • 79 篇 化学工程与技术
    • 70 篇 光学工程
    • 47 篇 信息与通信工程
    • 45 篇 航空宇航科学与技...
    • 42 篇 计算机科学与技术...
    • 37 篇 力学(可授工学、理...
    • 35 篇 软件工程
    • 32 篇 机械工程
    • 25 篇 环境科学与工程(可...
    • 19 篇 土木工程
    • 15 篇 交通运输工程
    • 14 篇 冶金工程
    • 14 篇 船舶与海洋工程
    • 12 篇 材料科学与工程(可...
    • 12 篇 控制科学与工程
    • 12 篇 建筑学
  • 16 篇 管理学
    • 12 篇 管理科学与工程(可...
  • 6 篇 农学
  • 1 篇 经济学
  • 1 篇 法学
  • 1 篇 医学

主题

  • 114 篇 stars
  • 77 篇 white dwarfs
  • 71 篇 galaxies
  • 69 篇 supernovae
  • 34 篇 gamma rays
  • 31 篇 photometry
  • 24 篇 luminance
  • 22 篇 mass transfer
  • 18 篇 binaries
  • 17 篇 active galactic ...
  • 13 篇 helium
  • 11 篇 pulsars
  • 11 篇 giant stars
  • 10 篇 surveys
  • 10 篇 stars:evolution
  • 10 篇 gravity waves
  • 9 篇 binaries: close
  • 8 篇 polarization
  • 8 篇 evolution
  • 8 篇 stars: evolution

机构

  • 510 篇 key laboratory f...
  • 456 篇 yunnan observato...
  • 281 篇 university of ch...
  • 223 篇 center for astro...
  • 123 篇 center for astro...
  • 120 篇 yunnan observato...
  • 120 篇 international ce...
  • 94 篇 key laboratory f...
  • 73 篇 school of astron...
  • 72 篇 key laboratory f...
  • 53 篇 key laboratory o...
  • 49 篇 key laboratory o...
  • 44 篇 tsinghua univers...
  • 42 篇 national astrono...
  • 42 篇 department of as...
  • 38 篇 department of as...
  • 38 篇 kavli institute ...
  • 35 篇 department of as...
  • 35 篇 cas key laborato...
  • 31 篇 key laboratory o...

作者

  • 60 篇 han zhanwen
  • 53 篇 chen xuefei
  • 52 篇 wang xiaofeng
  • 51 篇 zhang jujia
  • 48 篇 wang jiancheng
  • 36 篇 mao jirong
  • 30 篇 mo jun
  • 28 篇 sheng-bang qian
  • 26 篇 xiang danfeng
  • 25 篇 feng hai-cheng
  • 25 篇 li yan
  • 25 篇 wang bo
  • 22 篇 bai jin-ming
  • 21 篇 jin-ming bai
  • 21 篇 lu kai-xing
  • 21 篇 gu shenghong
  • 21 篇 wang jian-guo
  • 21 篇 brink thomas g.
  • 21 篇 yan shengyu
  • 21 篇 li wenxiong

语言

  • 772 篇 英文
  • 238 篇 其他
  • 2 篇 中文
检索条件"机构=kKey Laboratory for the Structure and Evolution of Celestial Objects"
1012 条 记 录,以下是421-430 订阅
排序:
Photometric Analysis of Asteroids in the Phocaea Region
收藏 引用
The Astronomical Journal 2025年 第1期170卷 35-35页
作者: Xiaoyun Xu Xiaobing Wang Karri Muinonen Shenghong Gu Antti Penttilä Fukun Xu Leilei Sun Jing Huang Pengfei Zhang Ao Wang Yunnan Observatories Chinese Academy of Sciences Kunming 650216 People’s Republic of China wangxb@*** University of Chinese Academy of Sciences Beijing 100049 People’s Republic of China Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming 650216 People’s Republic of China Department of Physics P.O. box 64 FI-00014 University of Helsinki Finland Center for Lunar and Planetary Sciences Institute of Geochemistry Chinese Academy of Sciences Guiyang People’s Republic of China Department of Physics Yuxi Normal University Yuxi 653100 People’s Republic of China
The Phocaea asteroid family, one of the large ancient families located in the inner main belt, may be the sources of near-Earth asteroids (NEAs) due to the nearby 3:1 mean motion resonance with Jupiter, the ν6 secula...
来源: 评论
A closer look at non-interacting he stars as a channel for producing the old population of type Ia supernovae
arXiv
收藏 引用
arXiv 2020年
作者: Liu, Zheng-Wei Stancliffe, Richard J. 396 Yangfangwang Guandu District Kunming650216 China Key Laboratory for the Structure and Evolution of Celestial Objects CAS Kunming650216 China Center for Astronomical Mega-Science CAS 20A Datun Road Chaoyang District Beijing100012 China Milne Centre for Astrophysics Department of Physics & Mathematics University of Hull HU6 7RX United Kingdom
The nature of the progenitors of type Ia supernovae (SNe Ia) remains a mystery. Binary systems consisting of a white dwarf (WD) and a main-sequence (MS) donor are potential progenitors of SNe Ia, in which a thermonucl... 详细信息
来源: 评论
High Velocity Runaway Binaries from Supernovae in Triple Systems
arXiv
收藏 引用
arXiv 2019年
作者: Gao, Yan Li, Jiao Jia, Shi Yunnan Observatories Chinese Academy of Sciences Kunming650011 China Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming650011 China University of Chinese Academy of Sciences
Recent studies on hypervelocity stars (HVSs) have generated a need to understand the high velocity limits of binary systems. If runaway binary systems with high movement speeds well in excess of 200km/s were to exist,... 详细信息
来源: 评论
Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
arXiv
收藏 引用
arXiv 2022年
作者: Zeng, Yaotian Liu, Zheng-Wei Heger, Alexander McCully, Curtis Röpke, Friedrich K. Han, Zhanwen Kunming650216 China Key Laboratory for the Structure and Evolution of Celestial Objects CAS Kunming650216 China University of Chinese Academy of Science Beijing100012 China Center for Astronomical Mega-Science CAS Beijing100012 China School of Physics and Astronomy Monash University 19 Rainforest Walk VIC3800 Australia Joint Institute for Nuclear Astrophysics National Superconducting Cyclotron Laboratory Michigan State University 1 Cyclotron Laboratory East LansingMI48824-1321 United States ClaytonVIC3800 Australia Stromlo ACT2611 Australia Las Cumbres Observatory 6740 Cortona Dr Ste 102 GoletaCA93117-5575 United States Department of Physics University of California Santa BarbaraCA93106-9530 United States Zentrum für Astronomie Universität Heidelberg Institut für Theoretische Astrophysik Philosophenweg 12 HeidelbergD-69120 Germany Heidelberger Institut für Theoretische Studien Schloss-Wolfsbrunnenweg 35 HeidelbergD-69118 Germany
Supernovae of Type Iax (SNe Iax) are an accepted faint subclass of hydrogen-free supernovae. Their origin, the nature of the progenitor systems, however, is an open question. Recent studies suggest that the weak defla... 详细信息
来源: 评论
Accreting CO material onto ONe white dwarfs towards accretion-induced collapse
收藏 引用
Research in Astronomy and Astrophysics 2018年 第3期18卷 121-128页
作者: Cheng-Yuan Wu Bo Wang Yunnan Observatories Chinese Academy of Sciences Kunming 650216 China Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming 650216 China University of Chinese Academy of Sciences Beijing 100049 China Center for Astronomical Mega-Science Chinese Academy of Sciences Beijing 100012 China
The final outcomes of accreting ONe white dwarfs(ONe WDs) have been studied for several decades,but there are still some issues that are not resolved. Recently,some studies suggested that the deflagration of oxygen ... 详细信息
来源: 评论
Cataclysmic variables based on the stellar spectral survey LAMOST DR3
收藏 引用
Research in Astronomy and Astrophysics 2018年 第6期18卷 67-88页
作者: Xianming L.Han Li-Yun Zhang Jian-Rong Shi Qing-Feng Pi Hong-Peng Lu Li-Bo Zhao Rachel K.Terheide Lin-Yang Jiang College of Physics/Department of Physics and Astronomy & Guizhou Provincial Key Laboratory of Public Big Data Guizhou University Dept.of Physics and Astronomy Butler University Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences National Astronomical Observatories Chinese Academy of Sciences Department of Astronomy Beijing Normal University
Big data in the form of stellar spectra from the spectroscopic survey associated with the Large Sky Area Multi-object Fiber Spectroscopic Telescope(LAMOST) are important for studying properties of cataclysmic variable... 详细信息
来源: 评论
Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-resolution Survey
收藏 引用
The Astrophysical Journal Supplement Series 2025年 第2期278卷 46-46页
作者: Sufen Guo Mikhail Kovalev Jiao Li Guoliang Lü Shi Jia Zhenwei Li Jiangdan Li Jianping Xiong Mingkuan Yang Tongyu He Xuefei Chen Zhanwen Han School of Physical Science and Technology Xinjiang University Urumqi 830046 People’s Republic of China Yunnan Observatories Chinese Academy of Sciences (CAS) Kunming 650216 People’s Republic of China lijiao@*** zhanwenhan@*** Key Laboratory for the Structure and Evolution of Celestial Objects CAS Kunming 650216 People’s Republic of China International Centre of Supernovae (ICESUN) Yunnan Key Laboratory of Supernova Research Yunnan Observatories Chinese Academy of Sciences (CAS) Kunming 650216 People’s Republic of China Key Laboratory of Optical Astronomy National Astronomical Observatories Chinese Academy of Sciences Beijing 100101 People’s Republic of China College of Physics Science and Technology Hebei University Baoding 071002 People’s Republic of China
The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital parameters remains limited. Utilizing the ...
来源: 评论
NSVS 01286630:a detached binary with a close-in companion
收藏 引用
Research in Astronomy and Astrophysics 2018年 第9期18卷 123-132页
作者: Bin Zhang Sheng-Bang Qian Nian-Ping Liu Wen-Ping Liao Li-Ying Zhu Ai-Jun Dong Qi-Jun Zhi Yunnan Observatories Chinese Academy of SciencesKunming 650216China Key Laboratory of the Structure and Evolution of Celestial Objects Chinese Academy of SciencesKunming 650216China University of Chinese Academy of Sciences Beijing 100049China School of Physics and Electronic Science Guizhou Normal UniversityGuiyang 550001China
New photometric observations of NS VS 01286630 were performed and two sets of fourcolor(B, V, Rc, Ic) light curves(LCs) were obtained. Using the 2013 version of the Wilson-Devinney(W-D) code, we analyzed these d... 详细信息
来源: 评论
High amplitude δ Scuti star BO Lyn with evidence of a late A-type companion in an elliptical orbit
收藏 引用
Research in Astronomy and Astrophysics 2018年 第1期18卷 119-126页
作者: Lin-Jia Li Sheng-Bang Qian Jia Zhang Li-Ying Zhu Wen-Ping Liao Yunnan Observatories Chinese Academy of Sciences Kunming 650216 China Key Laboratory of the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming 650216 China Center for Astronomical Mega-Science Chinese Academy of Sciences Beijing 100012 China University of Chinese Academy of Sciences Beijing 100049 China
We present 145 times of light maximum for high amplitude δ Scuti star BO Lyn based on several sky surveys(CRTS,DASCH,NSVS,OMC and Super WASP)and our photometric *** with the data in literature,a total of 179 times ... 详细信息
来源: 评论
Astronomical site monitoring system at lijiang observatory
arXiv
收藏 引用
arXiv 2020年
作者: Xin, Yu-Xin Bai, Jin-Ming Lun, Bao-Li Fan, Yu-Feng Wang, Chuan-Jun Liu, Xiao-Wei Yu, Xiao-Guang Ye, Kai Song, Teng-Fei Chang, Liang He, Shou-Sheng Mao, Ji-Rong Xu, Liang Xiong, Ding-Rong Zhang, Xi-Liang Wang, Jian-Guo Ding, Xu Feng, Hai-Cheng Liu, Xiang-Kun Huang, Yang Chen, Bing-Qiu Yunnan Observatories Chinese Academy of Sciences KunmingYunnan650216 China University of Chinese Academy of Sciences Beijing100049 China Key Laboratory for the Structure and Evolution of Celestial Objects Chinese Academy of Sciences Kunming650216 China Center for Astronomical Mega-Sciences Chinese Academy of Sciences Beijing100012 China South-Western Institute for Astronomy Research Yunnan University Kunming650500 China
We installed two sets of Astronomical Site Monitoring System(ASMS) at Lijiang Observatory(GMG), for the running of the 2.4-meter Lijiang optical telescope(LJT) and the 1.6-meter Multi-channel Photometric Survey Telesc... 详细信息
来源: 评论