2 citations · 2 across the 2 of their papers we have counts for
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Super-AGB stars: evolution and associated nucleosynthesis
M. L. Pumo, L. Siess, R. A. Zappala'
Based on evolutionary computations of 90 stellar models, we have analysed the impact of initial composition and core overshooting on the post-He-burning evolution and the associate…
Sources of uncertainties in the s-process in massive stars: convection and reaction rates
V. Costa, M. L. Pumo, A. Bonanno +1
Current models of s-nucleosynthesis in massive stars ( to ) are able to reproduce some main features of the abundance distributions of heavy i…
A search for very young Planetary Nebulae
G. Umana, L. Cerrigone, C. Trigilio +1
Despite numerous efforts, the transition from Asymptotic Giant Branch (AGB) stars to Planetary Nebulae (PN) is a poorly understood phase of stellar evolution. We have therefore car…
The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ?
V. Costa, M. Rayet, R. A. Zappalà +1
The most detailed calculations of the p-process call for its development in the O/Ne layers of Type II supernovae. In spite of their overall success in reproducing the solar system…