File:Alpha Arae.jpg

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Description
English: Artist's impression of the Be star Alpha Arae. The star is rotating with a velocity close to its break-up velocity and loses mass through a stellar wind emerging predominantly from the poles and reaching velocities of the order of 2000 km/s. The star is surrounded by a disc in Keplerian rotation.
Source http://www.eso.org/public/news/eso0635/
Author ESO/Anthony Meilland (Observatoire de la Côte dAzur, France)
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
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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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Date/TimeThumbnailDimensionsUserComment
current11:08, 14 February 2024Thumbnail for version as of 11:08, 14 February 20242,369 × 2,147 (1.03 MB)C messier (talk | contribs)full size
19:30, 16 September 2010Thumbnail for version as of 19:30, 16 September 20101,280 × 1,160 (274 KB)Sadalsuud~commonswiki (talk | contribs){{Information |Description={{en|1=Artist's impression of the Be star Alpha Arae. The star is rotating with a velocity close to its break-up velocity and loses mass through a stellar wind emerging predominantly from the poles and reaching velocities of the

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