Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …

We present the final sample of the Exploration of Local VolumE Satellites (ELVES) survey, a
survey of the dwarf satellites of a nearly volume-limited sample of Milky Way (MW)− like …

Abstract We use SDSS+ GALEX+ Galaxy Zoo data to study the quenching of star formation
in low-redshift galaxies. We show that the green valley between the blue cloud of star …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …

We introduce a set of high-resolution dissipationless simulations that model the Local Group
(LG) in a cosmological context: Exploring the Local Volume in Simulations (ELVIS). The …

We update van den Bergh's parallel-sequence galaxy classification in which S0 galaxies
form a sequence S0a–S0b–S0c that parallels the sequence Sa–Sb–Sc of spiral galaxies …

Using the latest cosmological hydrodynamic N-body simulations of groups and clusters, we
study how location in phase-space coordinates at z= 0 can provide information on …