File:Eso0304c.jpg

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DescriptionEso0304c.jpg	Türkçe: Template:İngThis image shows the general location of the newly discovered compact HII region with respect to a previously published Subaru Suprime-Cam image of NGC 4388. The image combines H-alpha narrow-band (hydrogen), O[III] narrow-band (oxygen), and broad-band optical V-band data. The extended pink filamentary structure in this image is due to gas ionized by the radiation from the nucleus of the galaxy. The vertical lines are caused by detector saturation of bright objects. The field of view is 11.6 x 5.0 arcmin2.
Date	16 Ocak 2003
Source	ESO http://www.eso.org/public/images/eso0304c/
Author	ESO
Permission (Reusing this file)	http://www.eso.org/public/outreach/copyright.html 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. CC BY 3.0 Creative Commons Attribution 3.0 truetrue

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	13:44, 6 July 2010		3,028 × 2,202 (2.41 MB)	CRea80 (talk \| contribs)	{{Bilgi \|açıklama={{İng}}This image shows the general location of the newly discovered compact HII region with respect to a previously published Subaru Suprime-Cam image of NGC 4388. The image combines H-alpha narrow-band (hydrogen), O[III] narrow-band

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