Supermassive black holes grow at the centre of galaxies in consonance with them. In this
Review Article, we discuss the mass-feeding mechanisms that lead to this growth in active …

Collisions and interactions between gas-rich galaxies are thought to be pivotal stages in
their formation and evolution, causing the rapid production of new stars, and possibly …

We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …

I use distance-and mass-limited subsamples of the Spitzer Survey of Stellar Structure in
Galaxies (S4G) to investigate how the presence of bars in spiral galaxies depends on mass …

We present the results of two-component (disc+ bar) and three-component (disc+ bar+
bulge) multiwavelength 2D photometric decompositions of barred galaxies in five Sloan …

Research over the past decade has shown diminishing evidence for major galaxy mergers
being a dominant mechanism for the growth of supermassive black holes (BHs) in galaxies …

Almost two-thirds of disk galaxies in the local universe host bars, which serve as important
drivers of secular evolutionary processes. While cosmological simulations are powerful tools …

Feedback from active galactic nuclei (AGNs) is expected to impact the amount of cold gas in
galaxies by driving strong galactic winds, by preventing external gas inflows, or by changing …

Observations in the local universe show a tight correlation between the masses of
supermassive black holes (SMBHs; M BH) and host-galaxy bulges (M bulge), suggesting a …

Feedback from active galactic nuclei (AGNs) has become established as a fundamental
process in the evolution of the most massive galaxies. Its impact on Milky Way (MW)-mass …