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

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Opis
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
Izvor http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-07c-00-fullres.jpg.html
Autor ESO
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Datum/vrijemeSmanjeni pregledDimenzijeKorisnikKomentar
trenutno22:51, 2 maj 2009Smanjeni pregled verzije na dan 22:51, 2 maj 20092.028 × 1.324 (2,19 MB)Fabian RRRR{{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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