منابع مشابه
Hot Bottom Burning in Asymptotic Giant Branch Stars and Its Effect on Oxygen Isotopic Abundances
A self-consistent calculation of asymptotic giant branch (AGB) evolution was carried out, including nucleosynthesis at the base of the convective envelope (hot bottom burning). Hot bottom burning was found to occur for stars between ~4.5 and ~7 M 0 , producing envelopes with 180/160 ;:S 106 and 103 ;:S 170jl 6 0 ;:5 101. The 170 abundance depends sensitively on the nuclear 170-destruction rate;...
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ژورنال
عنوان ژورنال: EAS Publications Series
سال: 2013
ISSN: 1633-4760,1638-1963
DOI: 10.1051/eas/1363002