File:Wiki Spect Binaries v2.gif

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Original file(1,460 × 1,018 pixels, file size: 165 KB, MIME type: image/gif, looped, 24 frames, 10 s)

Summary[edit]

Description
English: Two stars of different size orbiting the center of mass. The spectrum can be seen to split depending on the position and velocity of the stars. The shift of Star A is greater than that of Star B because the tangential velocity is higher. The line width of Star B is greater than that of Star A because the Star B is larger and more luminous.
Date
Source Own work
Author Primefac

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I, the copyright holder of this work, hereby publish it under the following licenses:
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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Date/TimeThumbnailDimensionsUserComment
current17:16, 7 December 2013Thumbnail for version as of 17:16, 7 December 20131,460 × 1,018 (165 KB)Primefac (talk | contribs){{Information |Description ={{en|1=Two stars of different size orbiting the center of mass. The spectrum can be seen to split depending on the position and velocity of the stars. The shift of Star A is greater than that of Star B because the tangent...
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