File:Phot-33b-03-fullres.jpg

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Summary

Description
English: Colour composite image of the starburst spiral galaxy NGC 1792 obtained with the FORS1 and FORS2 multi-mode instruments (at VLT MELIPAL and YEPUN, respectively). Its optical appearance of NGC 1792 is quite chaotic, due to the patchy distribution of dust throughout the disc of this galaxy. It is very rich in neutral hydrogen gas - fuel for the formation of new stars - and is indeed rapidly forming such stars. The galaxy is characterized by unusually luminous far-infrared radiation; this is due to dust heated by young stars. Note the numerous background galaxies in this sky field. North is up and East is to the left.

ID: phot-33b-03-fullres

Size: 2297x2306

Credit: ESO
Date Wed 07 Jan 2009 16:19:52 CET
Source

http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-33b-03-fullres.jpg.html

https://www.eso.org/public/images/eso0338b/
Author ESO

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Date/TimeThumbnailDimensionsUserComment
current21:27, 28 April 2009Thumbnail for version as of 21:27, 28 April 20092,297 × 2,306 (2.91 MB)Fabian RRRR{{Information |Description={{en|1=Colour composite image of the starburst spiral galaxy NGC 1792 obtained with the FORS1 and FORS2 multi-mode instruments (at VLT MELIPAL and YEPUN, respectively). Its optical appearance of NGC 1792 is quite chaotic, due to
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