The Chemical Yields of Stars in the Mass Range 9–15 M⊙
In M. Limongi et al. we presented and discussed the main evolutionary properties and final fate of stars in the mass range 7−15 M _⊙ . The evolutions of those models were computed by means of a medium-sized nuclear network that guaranteed a proper calculation of the nuclear energy generation and hen...
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| Hauptverfasser: | , , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
IOP Publishing
2025-01-01
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| Schriftenreihe: | The Astrophysical Journal Supplement Series |
| Schlagworte: | |
| Online-Zugang: | https://doi.org/10.3847/1538-4365/addf34 |
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