We study the scaling relations between gas-phase metallicity, stellar mass surface density
(Σ*), star formation rate surface density (ΣSFR), and molecular gas surface density () in local …

Context. Feedback from massive stars plays a crucial role in regulating the growth of young
star-forming galaxies (SFGs) and in shaping their interstellar medium (ISM). This feedback …

Local metal-poor galaxies stand as ideal laboratories for probing the properties of the
interstellar medium (ISM) in chemically unevolved conditions. Detailed studies of this …

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 the host galaxies of four apparently nonrepeating fast radio bursts (FRBs), FRB
20181223C, FRB 20190418A, FRB 20191220A, and FRB 20190425A, reported in the first …

Heavy element accumulation and stellar mass assembly are fundamental processes in the
formation and evolution of galaxies. However, the key elements that govern them, such as …

Stellar feedback-driven outflows regulate the stellar formation and chemical enrichment of
galaxies, yet the underlying dependence of mass outflow rate on galaxy properties remains …

Tidal interactions between galaxies often give rise to tidal tails, which can harbor
concentrations of stars and interstellar gas resembling dwarf galaxies. Some of these tidal …

Green Pea galaxies (GPs) present among the most intense starbursts known in the nearby
Universe. These galaxies are regarded as local analogs of high-redshift galaxies, making …

We present a catalogue of∼ 52 000 extragalactic H ii regions and their spectroscopic
properties obtained using Integral Field Spectroscopy (IFS) from MUSE observations. The …