Context. The study of galaxy formation and evolution critically depends on our
understanding of the complex photo-chemical processes that govern the evolution and …

The classical model of massive-star mechanical feedback is based on effects at solar
metallicity (Z⊙), yet feedback parameters are very different at low metallicity. Metal-poor …

Abstract We use the Hubble Space Telescope Advanced Camera for Surveys to obtain the
first spatially resolved, nebular imaging in the light of C iv λλ1548, 1551 by using the F150LP …

For the first time, the sulphur abundance relative to hydrogen (S/H) in the narrow-line
regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the …

Context. Lyman break analogs in the local Universe serve as counterparts to Lyman break
galaxies (LBGs) at high redshifts, which are widely regarded as major contributors to cosmic …

Context. Galactic winds determine how stellar feedback regulates the mass and metallicity of
galaxies. Observational studies show that galactic winds are multi-phase and magnetised. In …

Studying the galaxies responsible for reionization is often conducted through local
reionization-era analogs; however, many of these local analogs are too massive to be …

The new era of galaxy evolution studies hearkened in by JWST has led to the discovery of
z> 5 galaxies exhibiting excess nitrogen with log (N/O)~ 1 dex or more than expected from …

Feedback is widely recognized as an essential condition for Lyman continuum (LyC) escape
in star-forming galaxies. However, the mechanisms by which galactic outflows clear neutral …

Gas-phase chemical abundances are powerful probes of galactic evolutionary mechanisms:
the Interstellar Medium is enriched with the products of stellar nucleosynthesis, diluted by …