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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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-д хадгалсан:
Номзүйн дэлгэрэнгүй
Үндсэн зохиолчид: Marco Limongi, Lorenzo Roberti, Agnese Falla, Alessandro Chieffi, Ken’ichi Nomoto
Формат: Artigo
Хэл сонгох:Inglês
Хэвлэсэн: IOP Publishing 2025-01-01
Цуврал:The Astrophysical Journal Supplement Series
Нөхцлүүд:
Онлайн хандалт:https://doi.org/10.3847/1538-4365/addf34
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