Rotating massive main-sequence stars II. Simulating a population of LMC early B-type stars as a test of rotational mixing
| Data(s) |
2011
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|---|---|
| Resumo |
Context. Rotational mixing in massive stars is a widely applied concept, with far-reaching consequences for stellar evolution, nucleosynthesis, and stellar explosions. |
| Identificador | |
| Idioma(s) |
eng |
| Direitos |
info:eu-repo/semantics/restrictedAccess |
| Fonte |
Brott , I , Evans , C J , Hunter , I , De Koter , A , Langer , N , Dufton , P , Cantiello , M , Trundle , C , Lennon , D J , De Mink , S E , Yoon , S C & Anders , P 2011 , ' Rotating massive main-sequence stars II. Simulating a population of LMC early B-type stars as a test of rotational mixing ' Astronomy and Astrophysics , vol 530 , A116 . DOI: 10.1051/0004-6361/201016114 |
| Palavras-Chave | #/dk/atira/pure/subjectarea/asjc/3100/3103 #Astronomy and Astrophysics #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science |
| Tipo |
article |
