We compare stellar mass surface density, metallicity, age, and line-of-sight velocity
dispersion profiles in massive () present-day early-type galaxies (ETGs) from the MaNGA …

We investigate the kinematic properties of nine nearby early-type galaxies with evidence of
a disc-like component. Three of these galaxies are located in the field, five in the group, and …

Many processes have been proposed to explain the quenching of star formation in spiral
galaxies and their transformation into S0s. These processes affect the bulge and disc in …

The distribution of stellar metallicities within and across galaxies is an excellent relic of the
chemical evolution across cosmic time. We present a detailed analysis of spatially resolved …

Context. We study the spatially resolved properties of 343 elliptical galaxies with the
Mapping Nearby Galaxies at the Apache Point Observatory (MaNGA) survey. Aims. Our goal …

Gradients in the stellar populations (SP) of galaxies–eg in age, metallicity, stellar initial mass
function (IMF)–can result in gradients in the stellar-mass-to-light ratio, M*/L. Such gradients …

The relative roles of mergers and star formation in regulating galaxy growth are still a matter
of intense debate. We here present our decode, a new Discrete statistical sEmi-empiriCal …

The many unique properties of galaxies are shaped by physical processes that affect
different components of the galaxy–such as their bulges and discs–in different ways, and …

Lenticular (S0) galaxies are galaxies that exhibit a bulge and disc component, yet lack any
clear spiral features. With features considered intermediary between spirals and ellipticals …

We present the analysis of the full Mapping Nearby Galaxies at APO (MaNGA) DR17 sample
to characterize its population of compact galaxies. We focus on galaxies that fill the stellar …