File:Phot-18c-02.jpg

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Description
English: NGC 300, as seen through a narrow optical filter (H-alpha) in the red light of hydrogen atoms. A population of intrinsically bright and young stars turned "on" just a few million years ago. Their radiation and strong stellar winds have shaped many of the clouds of ionized hydrogen gas ("HII shells") seen in this photo. The "rings" near some of the bright stars are caused by internal reflections in the telescope.

ID: phot-18c-02

Press Release: 18/02

Object: NGC 300

Telescope: 2.2m

Instrument: WFI

Size: 5515x4475

Credit: ESO
Source http://www.eso.org/gallery/v/ESOPIA/Galaxies/phot-18c-02.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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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
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  • 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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current21:09, 2 May 2009Thumbnail for version as of 21:09, 2 May 20095,515 × 4,475 (13.56 MB)Fabian RRRR (talk | contribs){{Information |Description={{en|1=NGC 300, as seen through a narrow optical filter (H-alpha) in the red light of hydrogen atoms. A population of intrinsically bright and young stars turned "on" just a few million years ago. Their radiation and strong stel

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