We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …

Aims. The complexity of star formation at the physical scale of molecular clouds is not yet
fully understood. We investigate the mechanisms regulating the formation of stars in different …

Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …

We study the presence of optically-selected active galactic nuclei (AGNs) within a sample of
867 galaxies extracted from the extended Calar-Alto Legacy Integral Field spectroscopy …

Using a sample of∼ 15 000 kpc-scale star-forming spaxels in 28 galaxies drawn from the
ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we investigate the …

We present the second data release for the H i-MaNGA programme of H i follow-up
observations for the SDSS-IV MaNGA survey. This release contains measurements for 3669 …

Aims. The general consensus is that late-type galaxies undergo intense star-formation,
activity while early-type galaxies are mostly inactive. We question this general rule and …

GASP XXX. The Spatially Resolved SFR–Mass Relation in Stripping Galaxies in the Local
Universe - IOPscience This site uses cookies. By continuing to use this site you agree to our …

Abstract The ALMaQUEST (ALMA-MaNGA QUEnching and STar formation) survey is a
program with spatially resolved 12 CO (1− 0) measurements obtained with the Atacama …

We present a new characterization of the relations between star-formation rate, stellar mass,
and molecular gas mass surface densities at different spatial scales across galaxies (from …