We study the bar pattern speeds and corotation radii of 225 barred galaxies, using integral
field unit data from MaNGA and the Tremaine–Weinberg method. Our sample, which is …

ABSTRACT We have used Galaxy Zoo DECaLS (GZD) to study strong and weak bars in disc
galaxies. Out of the 314 000 galaxies in GZD, we created a volume-limited sample (0.01< z< …

We aim to unravel the interplay between bars, star formation (SF), and active galactic nuclei
(AGNs) in barred galaxies. To this end, we utilize the SDSS DR12 to select a sample of …

Improving our knowledge of global Milky Way (MW) properties is critical for connecting the
detailed measurements only possible from within our Galaxy to our understanding of the …

We study how bar strength and bar kinematics affect star formation in different regions of the
bar by creating radial profiles of EW [Hα] and D n 4000 using data from Sloan Digital Sky …

The challenge of consistent identification of internal structure in galaxies–in particular disc
galaxy components like spiral arms, bars, and bulges–has hindered our ability to study the …

We report evidence for star formation quenching in the central 8.6 kpc region of the jellyfish
galaxy JO201 that hosts an active galactic nucleus (AGN), while undergoing strong ram …

We present a study of barred galaxies in the cluster environment, exploiting a sample of
galaxies drawn from the extended WIde-field Nearby Galaxy-cluster Survey (OmegaWINGS) …

Context. Stellar bars are common morphological structures in the local Universe; according
to optical and NIR surveys, they are present in about two-thirds of disc galaxies. These …

Context. Stellar bars are known to gradually funnel gas to the central parts of disk galaxies. It
remains a matter of debate why the distribution of ionized gas along bars and in the …