I
I. Dominguez
Researcher at University of Granada
Publications - 65
Citations - 2382
I. Dominguez is an academic researcher from University of Granada. The author has contributed to research in topics: Stars & Nucleosynthesis. The author has an hindex of 21, co-authored 60 publications receiving 2239 citations.
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Journal ArticleDOI
Evolution, nucleosynthesis, and yields of low-mass asymptotic giant branch stars at different metallicities
Sergio Cristallo,Oscar Straniero,Roberto Gallino,Roberto Gallino,Luciano Piersanti,I. Dominguez,M. T. Lederer +6 more
TL;DR: In this paper, a model of low-mass AGB stars with metallicity ranging between Z = 0.0138 (the solar one) and Z= 0.0001, with a full nuclear network coupled to the stellar evolution code and a mass loss-period-luminosity relation is presented.
Journal ArticleDOI
Evolution, Nucleosynthesis, and Yields of Low-mass Asymptotic Giant Branch Stars at Different Metallicities. II. The FRUITY Database
Sergio Cristallo,Sergio Cristallo,Luciano Piersanti,Oscar Straniero,Roberto Gallino,Roberto Gallino,I. Dominguez,Carlos Abia,G. Di Rico,M. Quintini,Sara Bisterzo +10 more
TL;DR: The FRANEC Repository of Updated Isotopic Tables & Yields (FRUITY) as mentioned in this paper is a database dedicated to the nucleosynthesis of AGB stars, where users can freely download the full (from H to Bi) isotopic composition, as it changes after each third dredge-up (TDU) episode and the stellar yields the models produce.
Journal ArticleDOI
Evolution, nucleosynthesis and yields of low mass AGB stars
TL;DR: In this article, new models of low-mass AGB stars (2 Msun), with metallicity ranging between Z = 0.0138 (the solar one) and Z=0.0001, are presented.
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The 85Kr s-Process Branching and the Mass of Carbon Stars
TL;DR: In this paper, the authors present new spectroscopic observations for a sample of C(N)-type red giants, which belong to the class of asymptotic giant branch stars, experiencing thermal instabilities in the He-burning shell (thermal pulses), and show that carbon enrichment is accompanied by the appearance of s-process elements in the photosphere.
Journal ArticleDOI
The Kr85 s-process Branching and the Mass of Carbon Stars
TL;DR: In this paper, the authors present new spectroscopic observations for a sample of C(N)-type red giants, which belong to the class of Asymptotic Giant Branch stars, experiencing thermal instabilities in the He-burning shell (thermal pulses).