File:Star fission common envelope.png
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Size of this preview: 472 × 599 pixels. Other resolutions: 189 × 240 pixels | 378 × 480 pixels | 605 × 768 pixels | 807 × 1,024 pixels | 2,000 × 2,537 pixels.
Original file (2,000 × 2,537 pixels, file size: 185 KB, MIME type: image/png)
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Summary
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| 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'. |
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license.
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- to share – to copy, distribute and transmit the work
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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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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 (talk | contribs) | Compressed with pngout. Reduced by 148kB (44% decrease). |
| 17:13, 6 August 2012 |  | 2,000 × 2,537 (334 KB) | Marshallsumter (talk | contribs) |
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