File:Redrosedust wright f2000 smaller2.jpg

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Description

English: A close up view of the Rosette Nebula. The red color comes from Hydrogen. Spanish: Un primer plano de la Nebulosa Roseta. El color rojo se debe al hidrógeno. French: Gros plan de la nébuleuse Rosette. La couleur rouge vient de l'hydrogène.

Source

http://astro.ic.ac.uk/Research/Halpha/North/gallery.shtml - accessed 5/07,2007

Date

05/07/2007

Author

English: Image based on data obtained as part of the INT Photometric H-Alpha Survey of the Northern Galactic Plane, prepared by Nick Wright, University College London, on behalf of the IPHAS Collaboration French: Image basée sur des données acquises lors de la cartographie H-alpha du plan galactique nord par l'INT, préparée par Nick Wright, University College London, dans le cadre de la collaboration IPHAS.

Permission
(Reusing this file)

Disclaimer: These images are released into the public domain for private use or for use in the promotion of the IPHAS survey. If any image or images are redisplayed or reproduced, please accompany the image or images with the following acknowledgement: "Image based on data obtained as part of the INT Photometric H-Alpha Survey of the Northern Galactic Plane, prepared by Nick Wright, University College London, on behalf of the IPHAS Collaboration".


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Date/TimeThumbnailDimensionsUserComment
current19:30, 25 November 2008Thumbnail for version as of 19:30, 25 November 20081,680 × 1,050 (455 KB)Petero9 (talk | contribs){{Information |Description={{en|A close up view of the Rosette Nebula. The red color comes from Hydrogen.}} {{es|Un primer plano de la Nebulosa Roseta. El color rojo se debe al hidrógeno. }} {{fr|Gros plan de la nébuleuse Rosette. La couleur rouge vient
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