activity
20202026
most citedAlFoCS + Fornax3D: resolved star formation in the Fornax cluster with ALMA and MUSE

34 citations · 42 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Coupling between stellar and HI lopsidedness in Milky Way-type galaxies from the Auriga Superstars cosmological simulations

Arianna Dolfi, Facundo A. Gómez, Rebekka Bieri +5

Lopsidedness is common in disk galaxies, yet its origin and evolution remain unclear. Previous studies typically examined stellar and gas asymmetries separately, but a combined ana…

astro-ph.GA2025

XMAGNET : Kinetic, Thermal and Magnetic AGN Feedback in Massive Galaxies at Halo Masses M

Deovrat Prasad, Philipp Grete, Brian O'Shea +5

The interplay between radiative cooling of the circumgalactic medium (CGM) and feedback heating governs the evolution of the universe's most massive galaxies. This paper presents s…

astro-ph.GA2025

Stream Automatic Detection with Convolutional Neural Network (SAD-CNN)

Alex Vera-Casanova., Nicolas Monsalves Gonzalez, Facundo A. Gómez +8

Context. Galactic halos host faint substructures, such as stellar streams and shells, which provide insights into the hierarchical assembly history of galaxies. To date, such featu…

astro-ph.GA2024★ 8 cited

The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies

Elisa A. Tau, Antonela Monachesi, Facundo A. Gomez +7

The stellar halos of dwarf galaxies are becoming an object of interest in the extragalactic community due to their detection in some recent observations. Additionally, new cosmolog…

astro-ph.GA2020★ 34 cited

AlFoCS + Fornax3D: resolved star formation in the Fornax cluster with ALMA and MUSE

Nikki Zabel, Timothy A. Davis, Marc Sarzi +18

We combine data from ALMA and MUSE to study the resolved (~300 pc scale) star formation relation (star formation rate vs. molecular gas surface density) in cluster galaxies. Our sa…