566 citations · 8.8k across the 150 of their papers we have counts for
150 papers
On the encounter between the GASP galaxy JO36 and the radio plume of GIN 049
Alessandro Ignesti, Marisa Brienza, Benedetta Vulcani +15
We report on the serendipitous discovery of an unprecedented interaction between the radio lobe of a radio galaxy and a spiral galaxy. The discovery was made thanks to LOFAR observ…
The evolution of the cold gas fraction in nearby clusters ram-pressure stripped galaxies
Alessia Moretti, Paolo Serra, Cecilia Bacchini +8
Cluster galaxies are affected by the surrounding environment, which influences, in particular, their gas, stellar content and morphology. In particular, the ram-pressure exerted by…
The morphological transformation of ram pressure stripped galaxies: a pathway from late to early galaxy types
A. Marasco, B. M. Poggianti, J. Fritz +5
We investigate how the ageing of stellar populations can drive a morphological transformation in galaxies whose star formation (SF) activity has been quenched on short timescales,…
Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary results
Enrichetta Iodice, Michael Hilker, Goran Doll +23
Looking into the faintEst WIth MUSE (LEWIS) is an ESO large observing programme aimed at obtaining the first homogeneous integral-field spectroscopic survey of 30 extremely low-sur…
Simulated observations of star formation regions: infrared evolution of globally collapsing clouds
Jesús M. Jáquez-Domínguez, Roberto Galván-Madrid, Jacopo Fritz +6
The direct comparison between hydrodynamical simulations and observations is needed to improve the physics included in the former and test biases in the latter. Post-processing rad…
Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
Benedetta Vulcani, Tommaso Treu, Antonello Calabro +26
We combine JWST/NIRCam imaging and MUSE data to characterize the properties of galaxies in different environmental conditions in the cluster Abell2744 () and in its immed…