activity
19922025
most citedStar formation efficiency in galaxy interactions and mergers: a statistical study

474 citations · 1.9k across the 57 of their papers we have counts for

collaborators

56 papers

astro-ph.GA2025

Molecular gas in a system of two interacting galaxies overlapping on the line-of-sight

Anaëlle Halle, Barbara Mazzilli Ciraulo, Daniel Maschmann +2

Galaxy interactions can disturb gas in galactic discs, compress it, excite it, and enhance star formation. An intriguing system likely consisting of two interacting galaxies overla…

astro-ph.GA2025★ 1 cited

Investigating Galactic Fountains in M101: Insights from Ionized, UV emissions and Neutral Gas

Aashiya Anitha Shaji, Françoise Combes, Anne-Laure Melchior +1

Spiral galaxy disks are thought to exist in a quasi-stationary state, between fresh gas accretion from cosmic filaments and disk star formation, self-regulated through supernovae f…

astro-ph.GA2025★ 1 cited

Dynamical traction and black hole orbital migration

C. M. Boily, T. L. François, J. Freundlich +3

We investigate the circumstances which allow a black hole to remain put at the galactic centre when the stellar core is anisotropic. We use N-body calculations to study the respons…

astro-ph.GA2025

A group of merging galaxies falling onto Abell 2142

Aashiya Anitha Shaji, Anaëlle Hallé, Damir Gasymov +3

Galaxy clusters produce a very hostile environment to galaxies, whose gas gets stripped by ram-pressure, suffer galaxy interactions and witness quenching of their star formation. C…

astro-ph.GA2024★ 1 cited

Central kiloparsec region of Andromeda. I. Dynamical modelling

Lucie Cros, Françoise Combes, Anne-Laure Melchior +1

The Andromeda galaxy (M31) is the most nearby giant spiral galaxy, an opportunity to study with high resolution dynamical phenomena occurring in nuclear disks and bulges, able to e…

astro-ph.HE2024★ 2 cited

SN 1885A and supernova remnants in the centre of M31 with LOFAR

Deepika Venkattu, Peter Lundqvist, Miguel Pérez Torres +4

We present the first LOFAR image of the centre of M31 at a frequency of 150 MHz. We clearly detect three supernova remnants, which, along with archival VLA data at 3 GHz and other…