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20162022
most citedPartial mixing and the formation of 13C pockets in AGB stars: effects on the s-process elements

27 citations · 32 across the 3 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2022

The RADIOSTAR Project

Maria Lugaro, Benoit Côté, Marco Pignatari +12

Radioactive nuclei are the key to understanding the circumstances of the birth of our Sun because meteoritic analysis has proven that many of them were present at that time. Their…

astro-ph.SR2020

Nucleosynthetic yields of Z= intermediate-mass stars

P. Gil-Pons, C. L. Doherty, J. Gutiérrez +3

Abridged: Observed abundances of extremely metal-poor (EMP) stars in the Halo hold clues for the understanding of the ancient universe. Interpreting these clues requires theoretica…

astro-ph.SR2019

The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints

J. W. den Hartogh, R. Hirschi, M. Lugaro +5

Aims. We investigate the s-process during the AGB phase of stellar models whose cores are enforced to rotate at rates consistent with asteroseismology observations of their progeni…

astro-ph.SR2018

Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors

Pilar Gil-Pons, Carolyn L. Doherty, Jordi L. Gutiérrez +4

Abridged: Getting a better understanding of the evolution and nucleosynthetic yields of the most metal-poor stars (appr. Z<=10^-5) is critical because they are part of the big pict…

astro-ph.SR201727 cited

Partial mixing and the formation of 13C pockets in AGB stars: effects on the s-process elements

J. F. Buntain, C. L. Doherty, M. Lugaro +3

The production of the elements heavier than iron via slow neutron captures (the s process) is a main feature of the contribution of asymptotic giant branch (AGB) stars of low mass…

astro-ph.SR2016

Explosion of white dwarfs harboring hybrid CONe cores

E. Bravo, P. Gil-Pons, J. L. Gutiérrez +1

Recently, it has been found that off-centre carbon burning in a subset of intermediate-mass stars does not propagate all the way to the center, resulting in a class of hybrid CONe…