activity
20242026
collaborators

6 papers

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

The supersonic nature of jellyfish galaxies

Alessandro Ignesti, Francesca Loi, Antonino Marasco +20

All gas-rich galaxies in cluster environments are expected to experience ram-pressure stripping from the intra-cluster medium. However, only a fraction of these develop ongoing sta…

astro-ph.GA2025

Distinguishing ram pressure from gravitational interactions: Applying the Size-Shape Difference method to real galaxies

Augusto E. Lassen, Rory Smith, Benedetta Vulcani +12

In dense environments, mechanisms like ram pressure stripping (RPS) and gravitational interactions can induce similar morphological features in galaxies, distinguishable only throu…

astro-ph.GA2025

Star formation at different stages of ram-pressure stripping as observed through far-ultraviolet imaging of 13 GASP galaxies

Koshy George, B. M. Poggianti, B. Vulcani +12

Galaxies undergoing ram-pressure stripping develop gaseous tails that can extend several kiloparsecs outside the galaxy disc. We used far-ultraviolet and H imaging from the GAS…

astro-ph.GA2025

The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample

Bianca M. Poggianti, Benedetta Vulcani, Neven Tomicic +14

We present the full sample of 76 galaxies in 39 galaxy cluster fields at z=0.04-0.07 observed with VLT/MUSE by the GASP survey. Most of them (64) were observed as possible ram pres…

astro-ph.GA2024

Candidate ram-pressure stripped galaxies in six low-redshift clusters revealed from ultraviolet imaging

Koshy George, B. M. Poggianti, A. Omizzolo +12

The assembly of galaxy clusters is understood to be a hierarchical process with a continuous accretion of galaxies over time, which increases the cluster size and mass. Late-type g…