Determination of alpha spectroscopic factors for unbound 17O states
It has been recently suggested that hydrogen ingestion into the helium shell of massive stars could lead to high 13C and 15N excesses when the blast of a core collapse supernova (ccSN) passes through its helium shell. This prediction questions the origin of extremely high 13C and 15N abundances obse...
محفوظ في:
| المؤلفون الرئيسيون: | , , , , |
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| التنسيق: | Artigo |
| اللغة: | Inglês |
| منشور في: |
EDP Sciences
2017-01-01
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| سلاسل: | EPJ Web of Conferences |
| الوصول للمادة أونلاين: | https://doi.org/10.1051/epjconf/201716501022 |
| الوسوم: |
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