Hot Bottom Burning Nucleosynthesis in 6Msolar Stellar Models

Details Hot Bottom Burning Nucleosynthesis in 6Msolar Stellar Models Hot Bottom Burning Nucleosynthesis in 6Msolar Stellar Models

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..435l&link_type=abstract

Nuclear Physics A, v. 621, p. 435-438.

Physics

Nuclear Physics

6

Scientific paper

We present a brief summary of some nucleosynthesis calculations for 6 Msolar stellar models with metallicity Z = 0.02, 0.008, and 0.004. The calculations include Hot Bottom Burning. Our main results are the verification of earlier calculations of a super Li-rich phase, as well as substantial production of aluminium isotopes, especially at lower metallicities.

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