activity
20242026
collaborators

12 papers

astro-ph.GA2026

Gaia FGK benchmark stars: Abundances of n-capture elements of the third version

S. Vitali, P. Jofré, L. Casamiquela +10

In the current era, in which an unprecedented wealth of data are available for the study of the Milky Way, Gaia benchmark stars (GBSs) have become an established reference and cali…

astro-ph.SR2026

Stellar nucleosynthesis in the era of large surveys: S-process polluted binaries in GALAH DR4

A. Escorza, S. Vitali, D. Godoy-Rivera +11

Binary interactions during the AGB phase can lead to the formation of chemically peculiar stars with overabundances of s-process elements. Only a few hundreds of these stars have b…

astro-ph.GA2026

Reconstructing chemical enrichment pathways in disc galaxies: A phylogenetic approach

Brian Tapia-Contreras, Patricia B. Tissera, Emanuel Sillero +11

Phylogenetic methods, traditionally used in biology to trace the evolutionary relationships among species, are emerging as a powerful framework to reconstruct evolutionary processe…

astro-ph.GA2026

Disentangling chemical evolution histories with phylogenetic trees

Rebeca Canales, Paula Jofré, Claudia Aguilera-Gómez +6

Chemical abundances encode the fossil record of galaxy evolution in a complex and diverse way that requires innovative approaches to reconstruct galactic histories. We investigate…

astro-ph.SR2026

Gaia FGK Benchmark Stars: Impact of Spectral Resolution on Stellar Abundances

Ivanna Hernández-Araya, Claudia Aguilera-Gómez, Paula Jofré +5

In the era of large Milky Way spectroscopic surveys, calibrating and standardizing stellar parameters and abundance measurements is crucial. The Gaia benchmark stars (GBS) are key…

astro-ph.SR2026

Gaia FGK Benchmark Stars: Selecting Infrared Lines for Abundance Determination

Scarlet Elgueta, Paula Jofré, Claudia Aguilera-Gómez +7

The advent of new and more powerful infrared spectrographs has significantly motivated the advancement of the study of atomic and molecular line lists and stellar atmosphere models…