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王青德

维基百科,自由的百科全书

王青德(?),美国天文学家马萨诸塞大学阿默斯特分校教授。他的研究方向侧重于热星际介质星系际介质。1990年,他获得了哥伦比亚大学[1]博士学位。

奖项和荣誉

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出版物

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  • A Faint Discrete Source Origin for the Highly Ionized Iron Emission from the Galactic Centre Region, 2002, Nature 415, 148
  • Ultraluminous X-ray Source 1E 0953.8+6918 (M81 X-9): An Intermediate-Mass Black Hole Candidate and its Environs, 2002, MNRAS 332, 764
  • Chandra Observation of the Edge-on Galaxy NGC 3556 (M108): Violent Galactic Disk-Halo Interaction Revealed, 2003, ApJ 598, 969
  • Detection of X-ray-Emitting Hypernova Remnants in M101, 1999, ApJL, 517, 27
  • An Ultra Deep High Resolution X-ray Image of M101: X-ray Source Population in a Late-type Spiral, 1999, ApJ, 523, 121
  • Structure and Evolution of Hot Gas in 30 Doradus, 1999, ApJL, 510, 139

参考资料

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  1. ^ Wilford, John Noble. Is Star Spinning or Vibrating? Is It Even Real?. The New York Times. 4 April 1989: 13 [27 May 2011]. (原始内容存档于2018-11-27). 

外部链接

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