collaborators

13 papers

astro-ph.GA2026

ALMA CO-CAVITY II. Resolved Scaling Relations in Void Galaxies

S. B. De Daniloff, D. Espada, S. Duarte Puertas +22

Scaling relations involving star formation rates (SFRs), molecular gas mass, and stellar mass are key to understand galaxy evolution, and have previously been explored at resolved…

astro-ph.GA2026

Unveiling a cosmic tango: Integral field spectroscopy and numerical simulations of Arp 143's interaction

Hugo Martel, Carmelle Robert, Laurent Drissen +6

We present spectral data cubes of the interacting galaxy system Arp 143, composed of the ring galaxy NGC 2445 and the lenticular galaxy NGC 2444, obtained with the imaging Fourier…

astro-ph.GA2026

The Gas-Phase Mass-Metallicity Relation of Dwarf Galaxies Across Large-Scale Environments Using the CAVITY Parent Sample

Bahar Bidaran, Salvador Duarte Puertas, Isabel Pérez +13

The gas-phase mass-metallicity relation (MZR) of galaxies shows a noticeable break in slope and increased scatter at low stellar masses, suggesting that the physical processes gove…

astro-ph.GA2026

Galaxy groups within voids

M. Argudo-Fernández, G. Torres-Ríos, P. Vásquez-Bustos +18

In this work, we aim to identify and characterise a sample of galaxy groups within voids in the local Universe (z\,<\,0.08), taking into account the peculiarities of these vast and…

astro-ph.GA2026

ALMA CO-CAVITY I. Resolved Molecular Gas in Void Galaxies

D. Espada, S. B. De Daniloff, S. Duarte Puertas +21

The environment plays a key role in galaxy evolution, yet it remains unclear how detailed molecular gas properties and their connection to star formation and stellar content are in…

astro-ph.GA2026

Stellar mass and morphology segregation in pairs and multiplets in the cosmic web

G. Torres-Ríos, S. Verley, I. Pérez +4

In this work, we investigate whether the location of galaxies within the large-scale structures (LSS) of the Universe affects their stellar mass () and morphology. To this…