File:Star fission common envelope.png
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This is a file from the Wikimedia Commons. The description on its description page there is shown below.
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Summary
| Description |
English: This diagram suggests a reverse common envelope process for binary star formation. At some point in star formation, two cores, one for a main-sequence star (yellow) and the other for a red giant (gray) form within a common envelope. As mass transfer continues or decelerates, the red giant transfers to at or below its Roche lobe (dashed green line) and a partially stable binary is formed. |
| Date | |
| Source | The source is the Wikimedia Commons file, url=File:Common envelope diagram.svg. |
| Author | I rotated the figure 180°. The original authors are those listed in the url in 'Source'. |
Licensing
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
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File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:34, 1 October 2016 | | 2,000 × 2,537 (185 KB) | Cmdrjameson | Compressed with pngout. Reduced by 148kB (44% decrease). |
| 17:13, 6 August 2012 |  | 2,000 × 2,537 (334 KB) | Marshallsumter |
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