Monash Chemical Yields Project (Monχey) Element production in low- and intermediate-mass stars
نویسندگان
چکیده
منابع مشابه
New theoretical yields of intermediate mass stars
We present theoretical yields of H, 16 O for stars with initial masses between 0.8 and 8 M ⊙ and initial metallicities Z = 0.001, 0.004, 0.008, 0.02, and 0.04. We use the evolutionary tracks of the Geneva group up to the early asymptotic giant branch (AGB) in combination with a synthetic thermal-pulsing AGB evolution model to follow in detail the chemical evolution and mass loss up to the end o...
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Intermediate mass stellar evolution tracks from the main sequence to the tip of the AGB for five initial masses (2 to 6M⊙) and metallicity Z=0.0001 have been computed. The detailed 1D structure and evolution models include exponential overshooting, mass loss and a detailed nucleosynthesis network with updated nuclear reaction rates. The network includes a two-particle heavy neutron sink for app...
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We investigate the production of aluminium and the heavy magnesium isotopes in asymptotic giant branch (AGB) models. We evolve models with a wide range in initial mass (1 > (M⊙) > 6) and composition (Z = 0.02,0.008,0.004). We evolve the models from the pre-main sequence, through all intermediate stages including the core helium flash, to near the end of the thermally-pulsing AGB phase. We then ...
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ژورنال
عنوان ژورنال: Proceedings of the International Astronomical Union
سال: 2015
ISSN: 1743-9213,1743-9221
DOI: 10.1017/s1743921316004725