File:Ic443 wide - crop G189.6+3.3.jpg

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Ic443_wide_-_crop_G189.6+3.3.jpg (544 × 390 pixels, file size: 105 KB, MIME type: image/jpeg)

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Summary

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Description
English: crop of IC 443 wide field image. The stars η Geminorum, the diffuse emission from S249 (north), and the G189.6+3.3 partial shell (center) are visible.
Date 13 January 2008 (original upload date)
Source Credits: Giovanni Benintende.
Author The original uploader was Abdelqader at English Wikipedia.

Licensing

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GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.
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attribution share alike 		This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
You are free:
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  • 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.
  • share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
This licensing tag was added to this file as part of the GFDL licensing update.

Original upload log

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Transferred from en.wikipedia to Commons by Quadell using CommonsHelper.

The original description page was here. All following user names refer to en.wikipedia.
  • 2008-01-13 15:32 Abdelqader 800×539× (188221 bytes) Giovanni Benintende

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Date/TimeThumbnailDimensionsUserComment
current19:42, 8 September 2019Thumbnail for version as of 19:42, 8 September 2019544 × 390 (105 KB)Fabian RRRR (talk | contribs){{Information |Description={{en|crop of IC 443 wide field image. The stars η Geminorum, the diffuse emission from S249 (north), and the G189.6+3.3 partial shell (center) are visible.}} |Source=Credits: Giovanni Benintende. |Date={{original upload date|2008-01-13}} |Author={{original uploader|Abdelqader|wikipedia|en}} |Permission= |other_versions= }} == {{int:license-header}} == {{GFDL|migration=relicense}} == {{original upload log}} == {{transferred from|en.wikipedia|Quadell|CommonsHelper}}...

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