File:NGC1850.jpg
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DescriptionNGC1850.jpg | 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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Author | ESA, NASA and Martino Romaniello (European Southern Observatory, Germany) | |||
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current | 22:43, 27 July 2009 | 2,210 × 1,546 (3.79 MB) | Tryphon (talk | contribs) | Original size, from http://imgsrc.hubblesite.org/hu/db/images/hs-2001-25-a-full_jpg.jpg. | |
20:27, 3 August 2007 | 746 × 521 (127 KB) | Angusmclellan (talk | contribs) | {{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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