File:Wiki Spect Binaries v2.gif
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Summary
| 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 |
Licensing
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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/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:16, 7 December 2013 | | 1,460 × 1,018 (165 KB) | Primefac | {{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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