activity
20242026
collaborators

18 papers

astro-ph.GA2026

From blue to red spirals: Slow galaxy transformation via ram pressure stripping in TNG-50

V. Lora, J. I. Gonzalez-Carbajal, A. Pasquali +5

Late-type galaxies lose gas through ram-pressure stripping (RPS) after falling into a massive halo. Because this mechanism primarily removes the gaseous component while leaving the…

astro-ph.GA2026

Testing dark matter models and modified gravity theories with spatially resolved HI observations

Federico Lelli, Antonino Marasco, Timothy A. Davis +8

Understanding the nature of dark matter (DM) is one of the most pressing questions of modern physics. The flat rotation curves of galaxies, especially the extended HI rotation curv…

astro-ph.GA2026

An HI+radio continuum study of local cluster galaxies: Intercepting the early stages of environmental processing with MeerKAT

Alessandro Ignesti, Paolo Serra, Alessandro Bianchetti +14

The study uses MeerKAT HI 21 cm and 1.4 GHz radio continuum data to examine galaxies in three nearby clusters, revealing that early-stage environmental processing boosts star forma…

astro-ph.GA2026

AGN Feeding & Feedback Over the Galactic Scales

Filippo M. Maccagni, Vincenzo Mainieri, Isabella Prandoni +8

Active Galactic Nuclei (AGN) are key drivers of galaxy evolution, triggered by cold gas accreting onto a super-massive black hole. However, the processes regulating this gas accret…

astro-ph.GA2026

With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies

Augusto E. Lassen, Benedetta Vulcani, Jacopo Fritz +13

The environmental mechanisms driving unwinding spiral arms in cluster galaxies remain debated. While earlier studies attributed it mainly to gravitational interactions, recent work…

astro-ph.GA2026

Kinematic scaling relations of disc galaxies from ionised gas at and their connection with dark matter haloes

Pavel E. Mancera Piña, Enrico M. Di Teodoro, S. Michael Fall +3

We derive the Tully-Fisher (TFR, ) and Fall (FR, ) relations at redshift using a sample of 43 main-sequence disc galaxies with H