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r-process calculations and Galactic chemical evolution

โœ Scribed by Shinya Wanajo; Yuhri Ishimaru


Publisher
Elsevier Science
Year
2006
Tongue
English
Weight
666 KB
Volume
777
Category
Article
ISSN
0375-9474

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Low metallicity very massive stars with an initial mass between 140 M and 260 M can be subdivided into two groups: those between 140 M and 200 M which produce a relatively small amount of Fe, and those with a mass between 200 M and 260 M where the Fe-yield ejected during the supernova explosion is e