activity
20012025
most citedThe strong transformation of spiral galaxies infalling into massive clusters at z~0.2

170 citations · 782 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2025

Tracing Galaxy Evolution in infalling galaxies of Abell 496: From Starburst to Quenching

M. M. López-Gutiérrez, H. Bravo-Alfaro, P. T. Rahna +4

During the fall of late-type galaxies into clusters, they can experiment a variety of evolutionary mechanisms according their local environment. Consequently, studying the UV emiss…

astro-ph.GA2024★ 18 cited

Pre- and post-processing of cluster galaxies out to : The extreme case of A2670

Franco Piraino-Cerda, Yara L. Jaffé, Ana C. Lourenço +7

We study galaxy interactions in the large scale environment around A2670, a massive ( = ) and interacting galaxy cluster at…

astro-ph.GA2022★ 8 cited

Environmental cluster effects and galaxy evolution: The HI properties of the Abell clusters A85/A496/A2670

M. M. López-Gutiérrez, H. Bravo-Alfaro, J. H. van Gorkom +6

We study the impact of local environment on the transformation of spiral galaxies in three nearby () Abell clusters: A85/A496/A2670. These systems were observed in HI wit…

astro-ph.GA2021

HI gas, environment, and SF-quenching in the Abell clusters A85/A496/A2670

Martha M. López-Gutiérrez, Hector Bravo-Alfaro, Jacqueline H. van Gorkom +2

We study complete sample of spiral galaxies brighter than M-18.4 in three Abell clusters: A85 (0.055), A496 (0.033) and A2670 (0.076). This wo…

astro-ph.CO2021★ 22 cited

PACT. II. Pressure profiles of galaxy clusters using Planck and ACT

E. Pointecouteau, I. Santiago-Bautista, M. Douspis +9

The pressure of hot gas in groups and clusters of galaxies is a key physical quantity, which is directly linked to the total mass of the halo and several other thermodynamical prop…

astro-ph.GA2020★ 58 cited

The ram pressure stripped radio tails of galaxies in the Coma cluster

Hao Chen, Ming Sun, Masafumi Yagi +14

Previous studies have revealed a population of galaxies in galaxy clusters with ram pressure stripped (RPS) tails of gas and embedded young stars. We observed 1.4 GHz continuum and…