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描述 Located in the Large Magellanic Cloud, one of our neighboring dwarf galaxies, this young globular-like star cluster is surrounded by a pattern of filamentary nebulosity that is thought to have been created during supernova blasts. It consists of a main globular cluster in the center and a younger, smaller cluster, seen below and to the right, composed of extremely hot, blue stars and fainter, red T Tauri stars. This wide variety of stars allows a thorough study of star formation processes.
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作者 ESA, NASA and Martino Romaniello (European Southern Observatory, Germany)
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This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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当前2009年7月27日 (一) 22:432009年7月27日 (一) 22:43版本的缩略图2,210 × 1,546（3.79 MB）TryphonOriginal size, from http://imgsrc.hubblesite.org/hu/db/images/hs-2001-25-a-full_jpg.jpg.
2007年8月3日 (五) 20:272007年8月3日 (五) 20:27版本的缩略图746 × 521（127 KB）Angusmclellan{{Information |Description=Downloaded from http://hubblesite.org/gallery/album/entire_collection/pr2001025a/ |Source=Originally from [http://en.wikipedia.org en.wikipedia]; description page is/was [http://en.wikipedia.org/w/index.php?title=Image%3ANGC1850

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