File:Phot-07c-00-fullres.jpg

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Description
English: It is possible to follow the spiral structure of the Sombrero Galaxy almost all the way round. The dark areas around the stars and galaxies in the field are artefacts of the image processing. This galaxy is notable for its dominant nuclear bulge , composed primarily of mature stars, and its nearly edge-on disk composed of stars, gas, and intricately structured dust. The complexity of this dust, and the high resolution of this image, is most apparent directly in front of the bright nucleus, but is also very evident as dark absorbing lanes throughout the disk. A significant fraction of the galaxy disk is even visible on the far side of the source, despite its massive bulge.

ID: phot-07c-00

Press Photo: 07/00

Object: M 104

Instrument: FORS1

Size: 2028x1324

Credit: ESO
Source http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-07c-00-fullres.jpg.html
Author ESO
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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Under the following conditions:
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w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.

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current20:51, 2 May 2009Thumbnail for version as of 20:51, 2 May 20092,028 × 1,324 (2.19 MB)Fabian RRRR (talk | contribs){{Information |Description={{en|1=It is possible to follow the spiral structure of the Sombrero Galaxy almost all the way round. The dark areas around the stars and galaxies in the field are artefacts of the image processing. This galaxy is notable for it

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