NGC 604

NGC 604
星云
三角座星系內的NGC 604。
哈伯太空望遠鏡所見的
觀測資料: J2000 epoch
赤经01h 34m 33.2s[1]
赤纬+30° 47′ 06″[1]
距離2,700,000 光年   (840,000[2] 秒差距)
视星等 (V)+14.0 [1]
視尺度(V)1′.93 x 1′.2 arcmins[1]
星座三角座
物理性質
半径760[3] ly
絕對星等 (V)-13.8
值得注意的特徵大質量電離氫區
相關條目:星雲列表

NGC 604是位於三角座星系內的一個電離氫區,它是威廉·赫歇爾在1784年9月11日發現的。它是本星系團最大的電離氫區之一,距離地球約270萬光年,最長處的直徑約1,500光年(460秒差距),可見部分的大小是獵戶座大星雲的40倍,亮度則是6,300倍。如果在相同的距離上,它會如同金星般的明亮。像所有的發射星雲一樣,它的氣體被群聚在中心的大質量恆星電離[4]。這些恆星大約有200顆是O型星沃夫–瑞葉星,質量是105太陽質量,而年齡大約350萬歲[2]。不同於大麥哲倫星系蜘蛛星雲中心的星團(R136),NGC 604是一個更緊湊,更類似於巨大星協,原型的鱗狀排列星協(Scaled OB AssociationSOBA[5]

NASA/ESA哈伯太空望遠鏡提供了迄今最清晰的NGC 604的影像。

參考資料

  1. ^ 1.0 1.1 1.2 1.3 NASA/IPAC Extragalactic Database. Results for NGC 604. [2006-09-03]. (原始内容存档于2011-05-14). 
  2. ^ 2.0 2.1 Barba, Rodolfo. An in-depth analysis of a prototypical giant H II region: NGC 604. HST Proposal ID #10419. 2004. Bibcode:2004hst..prop.6732B. 
  3. ^ distance × sin( diameter_angle / 2 ) = 760 ly. radius
  4. ^ Astronomy Picture of the Day, November 2, 2000 NGC 604: Giant Stellar Nursery. NASA. [2007-02-10]. (原始内容存档于2007-02-05). 
  5. ^ Maíz-Apellániz, J.; Pérez, E.; Mas-Hesse, J. M. NGC 604, the Scaled OB Association (SOBA) Prototype. I. Spatial Distribution of the Different Gas Phases and Attenuation by Dust. The Astronomical Journal. 2004, 128 (3): 1196–1218. Bibcode:2004AJ....128.1196M. arXiv:astro-ph/0406130可免费查阅. doi:10.1086/422925. 
  • Some data in the table was updated from Sue French's column "Deep-sky Wonders", in the January 2006 issue of Sky & Telescope, p. 83.

外部連結

Template:Triangulum Galaxy

维基共享资源上的相關多媒體資源:NGC 604

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