Nucleosynthesis in rotating massive star
โ
N. Langer; J. Fliegner; A. Heger; S.E. Woosley
๐
Article
๐
1997
๐
Elsevier Science
๐
English
โ 567 KB
Observational evidence for rotationally induced mixing in massive stars is summarized. From these observations and the models required to explain them, we conclude that rotation will increase the primary metal yields of massive stars, enhance the production of H-burning secondary products (e.g. 14N