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南京大学天文与空间科学学院

最近,我校天文与空间科学学院丁明德教授课题组与美国蒙大拿州立大学物理系Dana Longcope教授课题组合作,在日冕加热机制研究方面取得重要进展,有关成果Observationally Quantified Reconnection Providing a Viable Mechanism for Active Region Coronal H. 自然 通讯 和 自然 天文学 报道我院张彬彬副教授、戴. 最近南京大学天文与空间科学学院张彬彬副教授、戴子高教授课题组在引力波事件及伽玛射线暴研究领域取得了重要进展,相关成果分别发表在近期的 自然通讯 和 自然天文学 杂志上。 最近,南京大学天文与空间科学学院行星课题组与北京大学科维理天文研究所等单位合作利用国家天文台的郭守敬望远镜 LAMOST 发现了一类新的太阳系外行星族群 热海星 Hoptunes。 自然 通讯 和 自然 天文. 报告题目 Tales of Intriguing AGN X-ray Variability as Threa. 时 间 2018年03月22日 15时00分. 时 间 2018年03月14日 10时30分.

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最近,我校天文与空间科学学院丁明德教授课题组与美国蒙大拿州立大学物理系Dana Longcope教授课题组合作,在日冕加热机制研究方面取得重要进展,有关成果Observationally Quantified Reconnection Providing a Viable Mechanism for Active Region Coronal H. 自然 通讯 和 自然 天文学 报道我院张彬彬副教授、戴. 最近南京大学天文与空间科学学院张彬彬副教授、戴子高教授课题组在引力波事件及伽玛射线暴研究领域取得了重要进展,相关成果分别发表在近期的 自然通讯 和 自然天文学 杂志上。 最近,南京大学天文与空间科学学院行星课题组与北京大学科维理天文研究所等单位合作利用国家天文台的郭守敬望远镜 LAMOST 发现了一类新的太阳系外行星族群 热海星 Hoptunes。 自然 通讯 和 自然 天文. 报告题目 Tales of Intriguing AGN X-ray Variability as Threa. 时 间 2018年03月22日 15时00分. 时 间 2018年03月14日 10时30分.
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南京大学天文与空间科学学院 | astronomy.nju.edu.cn Reviews

https://astronomy.nju.edu.cn

最近,我校天文与空间科学学院丁明德教授课题组与美国蒙大拿州立大学物理系Dana Longcope教授课题组合作,在日冕加热机制研究方面取得重要进展,有关成果Observationally Quantified Reconnection Providing a Viable Mechanism for Active Region Coronal H. 自然 通讯 和 自然 天文学 报道我院张彬彬副教授、戴. 最近南京大学天文与空间科学学院张彬彬副教授、戴子高教授课题组在引力波事件及伽玛射线暴研究领域取得了重要进展,相关成果分别发表在近期的 自然通讯 和 自然天文学 杂志上。 最近,南京大学天文与空间科学学院行星课题组与北京大学科维理天文研究所等单位合作利用国家天文台的郭守敬望远镜 LAMOST 发现了一类新的太阳系外行星族群 热海星 Hoptunes。 自然 通讯 和 自然 天文. 报告题目 Tales of Intriguing AGN X-ray Variability as Threa. 时 间 2018年03月22日 15时00分. 时 间 2018年03月14日 10时30分.

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南京大学天文与空间科学实践教育中心

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版权所有 南京大学天文与空间科学学院 技术支持 南京先极科技有限公司.

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Astroforum

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School of Astronomy and Space Science, NJU. Probing the cosmic expansion with redshift surveys: prospects and theoretical challenges. Star formation quenching in central and satellite galaxies. Puzzling accretion onto a black hole in M101 ULX-1. Magnetic Fields and Massive Star Formation. Black Holes Big and Small: Impact on Galaxy Formation. Cosmic Gas as a Probe of Structure Formation and Evolution. Quenching of Star Formation and 3D Spectroscopy of Nearby Galaxies. 李菂 研究员 国家天文台 2014年3月21日 周五 下午4 00.

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南京大学天文与空间科学学院学生园地

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南京大学现代天文与天体物理前沿研究暑期学校2010.8.8 - 8.18 南京

http://astronomy.nju.edu.cn/summer/summer/huan_ying.html

PREPARE FOR THE FUTURE!

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Doctor Forum, School of Astronomy and Space Science, Nanjing University

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School of Astronomy and Space Science, NJU. Dark Matter Indirect Detection and Gamma Ray Space Telescope. Magnification Relations of Singular Isothermal Quadrupole Lens and Perturbed by High-orders. Exploring Star Formation and Dust Attenuation of Galaxies Using Multiwavelength Data. Planetary crash: New insight into why hot Jupiters are so diverse. The source-lens clustering effect in the context of lensing tomography and its self-calibration. Modeling Non-equilbirum Collisional Plasmas. Recent observat...

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Revised kinematic distance calculator. Harvard-Smithsonian Center for Astrophysics, USA. Karl Menten (co-PI), Andreas Brunthaler (co-PI), Alberto Sanna, Jing Jing Li. Max-Planck-Institut für Radioastronomie, Germany. Nanjing University, China. Xu Ye, Hu Bo. Purple Mountain Observatory, China. Arcetri Observatory, Italy. National Astronomical Observatory of Japan. Torun Centre for Astronomy, Poland. University of Bielefeld, Germany. Korea Astronomy and Space Science Institute, South Korea.

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Chinese Astronomical Institutions----Institute of Atmospheric Physics Chinese Academy of Sciences

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Annual Meeting and Board of Directors. Research in Astronomy and Astrophysics. 90th Anniversary of the Foundation of CAS. IAU General Assembly, 2012 Beijing. 中国科学院国家天文台(National Astronomical Observatories(NAOC),Chinese Academy of Sciences (CAS). 地址 北京市朝阳区大屯路甲20号,邮政编码 100012,(Address 20A Datun Rd,Chaoyang District,Beiing 100012,P.R.China),Tel 010-64888708,Email goffice@nao.cas.cn,. Http:/ www.nao.cas.cn. 中科院云南天文台(Yunnan Astronomical Observatory, Chinese Academy of Sciences). 地址 南京市北京西路2号,邮政编码 210008,(Addr...

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ÓÑÇéÁ´½Ó

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1ÄÏ óÑ ÌìÎÄÑ Ïµ. 2Ææ µç ÓÎÄ â. 2001-2009 ðÁ ÐÇ éÖÆ.

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欢迎来到毫米波射电天文数据库

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格式 L B 半径 或hh:mm:ss.s dd:mm:ss.s 半径。 106796 5.312 10. 02:27:34.88 61:52:25.5 1.0. 18 53 19.00 01 14 35.0. Eg: OrionA or ORIONA,有坐标时不用源名. Eg: CO or CO(1-0) or 12CO. Eg: 2008 or 2008-10 or 2008-10-01. Email drlu@pmo.ac.cn. 版权所有 中国科学院紫金山天文台 备案序号 XXH12504-2-01. 技术支持 本数据库由中国科学院十二五信息化建设专项 科技数据资源整合与共享工程 项目提供支持.

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7. Everything Else - In Search of the Baiji - An Adventure in China

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4 Wuhan and Qi Qi. 6 Public Awareness of the Baiji. 9 Scenes from the River. 11 Update 1995: A Female Baiji. 12 Update 1999: Finless Porpoises. 13 Update 2003: Death of Qi Qi. 14 Update 2005: Ten-year Reunion. 15 Update 2007: Extinction? 16 Update 2010/2012: Five Year Review. 17 Update 2014: Flight of the Baiji. In Search of the Baiji: An Adventure in China. By D W. Hoard and S. Wachter. Telescopes, gymnastics, and kung fu). In Seattle. While we were in Nanjing. We discovered two men repairing a small te...

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About Me | Whistle Down The Wind ~

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Whistle Down The Wind. Astronomy is Life, others are just details. Happy in Astronomy, Everyday! Hi, I’m a graduate student from Department of Astronomy. I’m in the third year of my graduate life. My advisor is Prof. Qiusheng Gu. Right now, I’m a visiting student at Carnegie Observatories, Pasadena, CA, I’m working with Luis Ho on a project called Carnegie-Irvine Nearby Galaxies Survey. You can find my CV. 198607.22] I was born in Tianjin. 199209-1998.06] Studied in Yueyang Road Elementary School. 2004-2...

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Despre cutremure | INFP

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空间天气专业委员会

http://www.spaceweather.org.cn/links.htm

地址 中国科学院空间科学与应用研究中心 空间天气学国家重点实验室 北京市海淀区中关村南二条一号 邮编 100190. Email: xhzhao@spaceweather.ac.cn.

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Bo Zhang’s Homepage

http://bzhang.lamost.org/website

The universe is unfolding as it should. 好在2018年,哈勃的继任者 由美国国家航天局 NASA 、欧洲空间局 ESA 与加拿大宇航局 CSA 联手打造的詹姆斯 韦布空间望远镜 JWST 将搭乘阿丽亚娜5型运载火箭进入太空,并飞向150万千米之外环绕日地系统第二拉格朗日点的轨道,在那里远离地球与太阳的干扰,以空前高的灵敏度和精度窥探深空。 但除了精度、极限星等和覆盖天区之外,这些林林总总的星表之间有无明显的不一致之处 来自瑞典Uppsala大学的Beatriz Villarroel等人最近就比对了2003年发表的美国海军天文台B1.0 USNO-B1.0 星表以及后来的斯隆数字巡天 SDSS 数据,发现前者真的含有一个不存在SDSS对应体的星点。 虽说 Villarroel et al. (2016). 在可见光或近紫外波段,背照式CCD结合荧光涂层还可以在一定程度上克服这一不足 X射线波段又有搀杂硅 而非光学波段使用的半导体硅 来提升响应。 上周三,真相终于浮出了水面 这个现称 GW 151226. 8212; 下一页 ».

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南京大学天文与空间科学学院

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