The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

Optical spectroscopic measurements show that gas in dusty, starbursting galaxies known as
ultraluminous infrared galaxies (ULIRGs) in the local Universe has a significantly lower …

Context. In this work we study the stellar mass–metallicity relation (MZR) of an extended
sample of star-forming galaxies in the local Universe and its possible dependence on the …

Context. Void galaxies are essential for understanding the physical processes that drive
galaxy evolution because they are less affected by external factors than galaxies in denser …

We present deep, narrowband imaging of the nearby spiral galaxy M101 and its satellites to
analyze the oxygen abundances of their H ii regions. Using Case Western Reserve …

We conducted a long-slit spectrophotometry analysis to obtain the chemical abundances of
seven metal-poor H ii regions in three galaxies: UM 160, UM 420, and TOL 0513− 393. The …

We study the redshift evolution of the gas-phase O/H and N/O abundances, both (i) for
individual interstellar medium (ISM) regions within single spatially resolved galaxies and (ii) …

Exploiting the data from the GAs Stripping Phenomena in galaxies with MUSE (GASP)
survey, we study the gas-phase metallicity scaling relations of a sample of 29 cluster …

Within the standard model of hierarchical galaxy formation in a Λ cold dark matter universe,
the environment of galaxies is expected to play a key role in driving galaxy formation and …

We use the IllustrisTNG simulations to investigate the evolution of the mass–metallicity
relation (MZR) for star-forming cluster galaxies as a function of the formation history of their …