activity
20162026
most citedOn the SFR-M main sequence archetypal star-formation history and analytical models

133 citations · 788 across the 25 of their papers we have counts for

collaborators
Showing 2021Show all

9 papers · 1 filter

astro-ph.GA2021★ 18 cited

HI observations of the MATLAS dwarf and ultra-diffuse galaxies

Melina Poulain, Francine R. Marleau, Rebecca Habas +8

The presence of HI gas in galaxies is inextricably linked to their morphology and evolution. This paper aims to understand the HI content of the already identified 2210 dwarfs loca…

astro-ph.GA2021

Origin of the spectacular tidal shells of galaxy NGC474

Michal Bílek, Jérémy Fensch, Ivana Ebrová +4

The lenticular galaxy NGC474 hosts a rich system of tidal shells and streams, some of which are exceptionally bright. Two teams recently presented spectroscopic observations of the…

astro-ph.GA2021★ 64 cited

Ultra diffuse galaxies in the MATLAS low-to-moderate density fields

Francine R. Marleau, Rebecca Habas, Melina Poulain +10

Recent advances in deep dedicated imaging surveys over the past decade have uncovered a surprisingly large number of extremely faint low surface brightness galaxies with large phys…

astro-ph.GA2021★ 12 cited

Stellar feedback in a clumpy galaxy at 3.4

E. Iani, A. Zanella, J. Vernet +18

Giant star-forming regions (clumps) are widespread features of galaxies at . Theory predicts that they can play a crucial role in galaxy evolution if they survive to…

astro-ph.GA2021★ 67 cited

Structure and morphology of the MATLAS dwarf galaxies and their central nuclei

Melina Poulain, Francine R. Marleau, Rebecca Habas +10

We present a photometric study of the dwarf galaxy population in the low to moderate density environments of the MATLAS (Mass Assembly of early-Type gaLAxies with their fine Struct…

astro-ph.GA2021★ 19 cited

Hierarchical fragmentation in high redshift galaxies revealed by hydrodynamical simulations

Baptiste Faure, Frédéric Bournaud, Jérémy Fensch +4

High-redshift star-forming galaxies have very different morphologies compared to nearby ones. Indeed, they are often dominated by bright star-forming structures of masses up to $10…