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Summary
| Description |
English: Supernovae types as a function of initial mass and initial content of elements heavier than helium (metallicity) |
| Date | |
| Source | Own work based on A. Heger, C. L. Fryer, S. E. Woosley, N. Langer, D. H. Hartmann: How massive single stars end their life. The Astrophysical Journal, 591:288–300, 2003 July 1 |
| Author | Fulvio314 |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:07, 16 April 2020 | | 512 × 324 (5 KB) | Jarvisa | Simplified SVG source |
| 10:24, 28 November 2013 |  | 512 × 324 (339 KB) | Fulvio314 | =={{int:filedesc}}== {{Information |description={{en|1=Supernovae types as a function of initial mass and initial content of elements heavier than Helium (metallicity)}} |date=2013-11-28 11:00:00 |source={{own}} based on [http://iopscience.iop.org/0004... |
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