activity
20152026
most citedGrids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

101 citations · 870 across the 50 of their papers we have counts for

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Showing 2024Show all

5 papers · 1 filter

astro-ph.SR2024

Production of Lithium and Heavy Elements in AGB Stars Experiencing PIEs

A. Choplin, L. Siess, S. Goriely +1

Asymptotic giant branch (AGB) stars can experience proton ingestion events (PIEs), leading to a rich nucleosynthesis. During a PIE, the intermediate neutron capture process (i-proc…

astro-ph.SR2024

Proton ingestion in asymptotic giant branch stars as a possible explanation for J-type stars and AB2 grains

A. Choplin, L. Siess, S. Goriely

J-type stars are a subclass of carbon stars that are generally Li-rich, not enriched in s-elements, and have low C/C ratios. They were suggested to be the manufacture…

astro-ph.SR2024★ 24 cited

Rapidly rotating Population III stellar models as a source of primary nitrogen

Sophie Tsiatsiou, Yves Sibony, Devesh Nandal +12

The first stars might have been fast rotators. This would have important consequences for their radiative, mechanical and chemical feedback. We discuss the impact of fast initial r…

astro-ph.SR2024★ 12 cited

Massive stars evolution with new C12+C12 nuclear reaction rate -- the core carbon-burning phase

T. Dumont, E. Monpribat, S. Courtin +7

Nuclear reactions drive the stellar evolution and contribute to the stellar and galactic chemicals abundances. New determinations of the nuclear reaction rates for key fusion react…

astro-ph.SR2024

The intermediate neutron capture process. V. The i-process in AGB stars with overshoot

A. Choplin, L. Siess, S. Goriely +1

The intermediate neutron capture process (i-process) can develop during proton ingestion events (PIE), potentially during the early stages of low-mass low-metallicity asymptotic gi…