71 citations · 325 across the 10 of their papers we have counts for
21 papers · 1 filter
Central kinematics of the Galactic globular cluster M80
Fabian Göttgens, Sebastian Kamann, Holger Baumgardt +7
We use spectra observed with the integral-field spectrograph MUSE to reveal the central kinematics of the Galactic globular cluster Messier 80 (M80, NGC 6093). Using observations o…
On the assembly history of massive galaxies. A pilot project with VEGAS deep imaging and M3G integral field spectroscopy
Marilena Spavone, Davor Krajnović, Eric Emsellem +2
In this paper we present the new deep images from the VEGAS survey of three massive (~M) galaxies from the MUSE Most Massive Galaxies (M3G) project, w…
The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
Nicolas F. Bouché, Shy Genel, Alisson Pellissier +14
We investigate the specific angular momentum (sAM) profiles of intermediate redshift () star-forming galaxies (SFGs) in the relatively unexplored regime of low…
The Tully-Fisher relation in dense groups at in the MAGIC survey
Valentina Abril-Melgarejo, Benoît Epinat, Wilfried Mercier +11
Galaxies in dense environments are subject to interactions and mechanisms which directly affect their evolution by lowering their gas fractions and reducing their star-forming capa…
The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
Sebastiaan L. Zoutendijk, Jarle Brinchmann, Nicolas F. Bouché +5
Aims. We use stellar line-of-sight velocities to constrain the dark matter-density profile of Eridanus 2, an ultra-faint dwarf galaxy (, $M_* \approx 9 \times…
Census and classification of low-surface-brightness structures in nearby early-type galaxies from the MATLAS survey
Michal Bílek, Pierre-Alain Duc, Jean-Charles Cuillandre +9
The morphology of galaxies gives essential constraints on the models of galaxy evolution. The morphology of the features in the low-surface-brightness regions of galaxies has not b…