Within the Local Universe galaxies can be studied in great detail star by star, and here we
review the results of quantitative studies in nearby dwarf galaxies. The color-magnitude …

ABSTRACT The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies
using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic …

Positional, structural, and dynamical parameters for all dwarf galaxies in and around the
Local Group are presented, and various aspects of our observational understanding of this …

We extend the PARSEC library of stellar evolutionary tracks by computing new models of
massive stars, from 14 to 350 M⊙. The input physics is the same used in the PARSEC V1. 1 …

We present a new set of high-resolution hydrodynamic cosmological zoom-in simulations
that apply the Feedback In Realistic Environments physics to both Local Group (LG)-like and …

ABSTRACT We present LITTLE THINGS (Local Irregulars That Trace Luminosity Extremes,
The H i Nearby Galaxy Survey), which is aimed at determining what drives star formation in …

We measured velocities of 862 individual red giant stars in seven isolated dwarf galaxies in
the Local Group: NGC 6822, IC 1613, VV 124 (UGC 4879), the Pegasus dwarf irregular …

Context. We present new photometric data from our Herschel guaranteed time key
programme, the Dwarf Galaxy Survey (DGS), dedicated to the observation of the gas and …

ABSTRACT We use archival Hubble Space Telescope observations of resolved stellar
populations to derive the star formation histories (SFHs) of 18 nearby starburst dwarf …

The starburst phenomenon can shape the evolution of the host galaxy and the surrounding
intergalactic medium. The extent of the evolutionary impact is partly determined by the …