collaborators

6 papers

astro-ph.GA2025

Bar ages derived for the first time in nearby galaxies: Insights on secular evolution from the TIMER sample

Camila de Sá-Freitas, Dimitri A. Gadotti, Francesca Fragkoudi +9

Once galaxies settle their discs and become self-gravitating, stellar bars can form, driving the subsequent evolution of their host galaxy. Determining the ages of bars can therefo…

astro-ph.GA2025

The resolved star-formation efficiency of early-type galaxies

Thomas G. Williams, Francesco Belfiore, Martin Bureau +19

Understanding how and why star formation varies between galaxies is fundamental to our comprehension of galaxy evolution. In particular, the star-formation efficiency (SFE; star-fo…

astro-ph.GA2025

The puzzle of isolated and quenched dwarf galaxies in cosmic voids

Bahar Bidaran, Isabel Pérez, Laura Sánchez-Menguiano +12

We report, for the first time, the detection of a sample of quenched and isolated dwarf galaxies (with 8.9 log(M/M) 9.5) in the least dense regi…

astro-ph.GA2024

CAVITY: Calar Alto Void Integral-field Treasury surveY. I. First public data release

Rubén García-Benito, Andoni Jiménez, Laura Sánchez-Menguiano +40

The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most under-dense…

astro-ph.GA2024

Dynamical resonances in PHANGS galaxies

Marina Ruiz-García, Miguel Querejeta, Santiago García-Burillo +13

Bars are remarkable stellar structures that can transport gas toward centers and drive the secular evolution of galaxies. In this context, it is important to locate dynamical reson…

astro-ph.GA2024

The effect of local and large scale environment on the star formation histories of galaxies

G. Torres-Ríos, I. Pérez, S. Verley +15

We aim to investigate how the local environment influences the star formation history (SFH) of galaxies residing in various large-scale environments. We categorise a sample of 9384…