Gas inflow feeds galaxies with low-metallicity gas from the cosmic web, sustaining star
formation across the Hubble time. We make a connection between these inflows and …

Models of galaxy formation predict that gas accretion from the cosmic web is a primary driver
of star formation over cosmic history. Except in very dense environments where galaxy …

Extremely metal poor (XMP) galaxies are known to be very rare, despite the large numbers
of low-mass galaxies predicted by the local galaxy luminosity function. This paper presents a …

We present a new derivation of the star formation history (SFH) of the dSph galaxy Fornax in
two central regions, characterized by unprecedented precision and age resolution. It reveals …

We measure the environmental dependence, where environment is defined by the distance
to the third nearest neighbor, of multiple galaxy properties inside the Environmental COntext …

Context. It has been proposed that mergers induce starbursts and lead to important
morphological changes in galaxies. Most studies so far have focused on large galaxies, but …

A clear link between a dwarf–dwarf merger event and enhanced star formation (SF) in the
recent past was recently identified in the gas-dominated merger remnant VCC 848, offering …

We present optical photometry of Hubble Space Telescope (HST) Advanced Camera for
Surveys (ACS)/Wide Field Camera (WFC) data of the resolved stellar populations in the …

Abstract Using VIsible MultiObject Spectrograph (VIMOS)-integral field unit (IFU)
observations, we study the interstellar medium (ISM) of two star-forming dwarf galaxies, UM …

We present high-spatial-resolution (∼ 0 farcs 2, or∼ 3 pc) CO (2–1) observations of the
nearest young starburst dwarf galaxy, NGC 5253, taken with the Atacama Large Millimeter …