International audienceWe use a sample of z = 0 galaxies visually classified as slow rotators (SRs) in the EAGLE hydrodynamical simulations to explore the effect of galaxy mergers on their formation, characterize their intrinsic galaxy properties, and study the connection between quenching and kinematic transformation. SRs that have had major or minor mergers (mass ratios ≥0.3 and 0.1-0.3, respectively) tend to have a higher triaxiality parameter and ex-situ stellar fractions than those that had exclusively very minor mergers or formed in the absence of mergers ('no-merger' SRs). No-merger SRs are more compact, have lower black hole-to-stellar mass ratios and quenched later than other SRs, leaving imprints on their z = 0 chemical composition...
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within t...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...
In this Letter, we investigate the impact of environment on integrated and spatially resolved stella...
International audienceWe use a sample of z = 0 galaxies visually classified as slow rotators (SRs) i...
Abstract We use a sample of z = 0 galaxies visually classified as slow rotators (SRs) in the eagle h...
Recent observations from integral field spectroscopy (IFS) indicate that the fraction of galaxies th...
International audienceContext. Early-type galaxies (ETGs) are divided into slow and fast rotators (F...
International audienceTwo-dimensional integral field surveys such as ATLAS3D are producing rich obse...
International audienceWe study the evidence for a diversity of formation processes in early-type gal...
We study the formation of early-type galaxies (ETGs) through mergers with a sample of 70 high-resolu...
Context. Numerical studies have shown that the properties of the S0 galaxies with kinemati...
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within t...
Context. Numerical studies have shown that the properties of the S0 galaxies with kinematics interme...
We study the formation of early-type galaxies (ETGs) through mergers with a sample of 70 high-resolu...
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry suggested a p...
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within t...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...
In this Letter, we investigate the impact of environment on integrated and spatially resolved stella...
International audienceWe use a sample of z = 0 galaxies visually classified as slow rotators (SRs) i...
Abstract We use a sample of z = 0 galaxies visually classified as slow rotators (SRs) in the eagle h...
Recent observations from integral field spectroscopy (IFS) indicate that the fraction of galaxies th...
International audienceContext. Early-type galaxies (ETGs) are divided into slow and fast rotators (F...
International audienceTwo-dimensional integral field surveys such as ATLAS3D are producing rich obse...
International audienceWe study the evidence for a diversity of formation processes in early-type gal...
We study the formation of early-type galaxies (ETGs) through mergers with a sample of 70 high-resolu...
Context. Numerical studies have shown that the properties of the S0 galaxies with kinemati...
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within t...
Context. Numerical studies have shown that the properties of the S0 galaxies with kinematics interme...
We study the formation of early-type galaxies (ETGs) through mergers with a sample of 70 high-resolu...
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry suggested a p...
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within t...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...
In this Letter, we investigate the impact of environment on integrated and spatially resolved stella...