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20012025
most citedSuper and massive AGB stars - IV. Final fates - Initial to final mass relation

261 citations · 1.2k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2025

An AGB star as the source of the abundance pattern of hyper-metal-poor star HE 1327-2326

P. Gil-Pons, S. W. Campbell, C. L. Doherty +1

Abridged. HE 1327-2326 (HE 1327), with [Fe/H]=-5.2, is one of the most metal-poor stars detected and a candidate to be the offspring of the first stars. Numerous efforts have been…

astro-ph.SR2023★ 16 cited

Carbon-oxygen ultra-massive white dwarfs in general relativity

Leandro G. Althaus, Alejandro H. Córsico, María E. Camisassa +4

We employ the La Plata stellar evolution code, LPCODE, to compute the first set of constant rest-mass carbon-oxygen ultra-massive white dwarf evolutionary sequences for masses high…

astro-ph.SR2022★ 9 cited

Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars

P. Gil-Pons, C. L. Doherty, S. W. Campbell +1

Abridged. We aim to better characterise the evolution and fates, and determine updated nucleosynthetic yields of intermediate-mass stars between primordial and EMP metallicity (Z=1…

astro-ph.GA2022

Primordial black holes capture by stars and induced collapse to low-mass stellar black holes

Marc Oncins, Jordi Miralda-Escudé, Jordi L. Gutiérrez +1

Primordial black holes in the asteroid-mass window ( to ), which might constitute all the dark matter, can be captured by stars when they tra…

astro-ph.SR2020★ 15 cited

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.SR2018★ 18 cited

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…