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20072018
most citedSuper and massive AGB stars - IV. Final fates - Initial to final mass relation

261 citations · 1.1k across the 18 of their papers we have counts for

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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…

astro-ph.SR2014★ 261 cited

Super and massive AGB stars - IV. Final fates - Initial to final mass relation

Carolyn L. Doherty, Pilar Gil-Pons, Lionel Siess +2

We explore the final fates of massive intermediate-mass stars by computing detailed stellar models from the zero age main sequence until near the end of the thermally pulsing phase…

astro-ph.SR2014★ 8 cited

Numerical Tests of Rotational Mixing in Massive Stars with the new Population Synthesis Code BONNFIRES

Herbert H. B. Lau, Robert G. Izzard, Fabian R. N. Schneider

We use our new population synthesis code BONNFIRES to test how surface abundances predicted by rotating stellar models depend on the numerical treatment of rotational mixing, such…

astro-ph.SR2014★ 188 cited

BONNSAI: a Bayesian tool for comparing stars with stellar evolution models

Fabian R. N. Schneider, Norbert Langer, Alex de Koter +3

Powerful telescopes equipped with multi-fibre or integral field spectrographs combined with detailed models of stellar atmospheres and automated fitting techniques allow for the an…

astro-ph.SR2014★ 120 cited

Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z=0.001 and 0.0001

Carolyn L. Doherty, Pilar Gil-Pons, Herbert H. B. Lau +3

We present a new grid of stellar models and nucleosynthetic yields for super-AGB stars with metallicities Z=0.001 and 0.0001, applicable for use within galactic chemical evolution…

astro-ph.SR2013★ 1 cited

Modelling binary rotating stars by new population synthesis code BONNFIRES

Herbert H. B. Lau, Robert G. Izzard, Fabian R. N. Schneider

BONNFIRES, a new generation of population synthesis code, can calculate nuclear reaction, various mixing processes and binary interaction in a timely fashion. We use this new popul…