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NGC 2467

维基百科,自由的百科全书
欧洲南方天文台拍摄的NGC 2467

NGC 2467是一个恒星形成区域,俗称“骷髅头星云”,[1]其外观偶尔也被比喻为色彩丰富的山魈。它包括含有大量氢气的区域,产生新的恒星。[2]它是特伦斯·迪金森著作《哈勃的宇宙:最伟大的发现和最新画面》(Hubble’s Universe: Greatest Discoveries and Latest Images)一书中被作为特色描述的区域之一。[3] [nb 1]

NGC 2467曾长期被认为是船尾座的核心。然而,NGC 2467并不指一个特殊的开放星群,[4]其实,它是由几个具有明显不同的距离和明显不同的径向速度的恒星组叠加在一起,这些恒星组在视线上大致在同一条线上。[5]


脚注

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  1. ^ An annotated image at Commons assists in understanding the following discussion.

参考资料

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  1. ^ Jeff Barbour; Tammy Plotner. What's Up 2006 - 365 Days of Skywatching. Lulu. : 81 [2013-03-04]. (原始内容存档于2014-08-12). 
  2. ^ A cosmic concoction in NGC 2467. Space Telescope. [February 28, 2013]. (原始内容存档于2019-05-08). 
  3. ^ Stunning Gallery of Previously Unpublished Images - Universe Today. [2013-03-04]. (原始内容存档于2012-12-09). 
  4. ^ Lodén, L. O. A study of NGC 2467 and the association Pup I. Arkiv för Astronomii. 1966, 4: 65–72 [24 February 2013]. (原始内容存档于2019-09-30). 
  5. ^ Pişmiş, P.; Moreno, M. A. Internal motions in H II regions. III. The nebular complex NGC 2467. Revista Mexicana de Astronomia y Astrofisica. 1976, 1: 373–380 [24 February 2013]. (原始内容存档于2019-12-07). 

参见

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外部链接

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