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20212026
most citedGalaxy Zoo: Stronger bars facilitate quenching in star forming galaxies

56 citations · 64 across the 11 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA20261 cited

The complex relationships between AGN, bars and bulges

Izzy L. Garland, Henry Best, Lucy F. Fortson +9

Context. Via scaling relations, it is well-known that active galactic nuclei (AGN) and bulges are linked. This link was thought to be driven by mergers, but recent studies show tha…

astro-ph.GA20261 cited

The effects of bar strength and kinematics on galaxy evolution II: The global and local impacts of slow-strong bars

Petra Mengistu, Karen L. Masters, Tobias Geron +3

There is now clear evidence, from a variety of studies, that galactic bars contribute to and/or accelerate processes which quench galaxies. However, bars have a variety of strength…

astro-ph.GA2025

Strong Bars, Strong Inflow: The Effect of Bar Strength on Gas Inflow

Maelle Magnan, Tobias Geron, Izzy L. Garland +5

Stellar bars are elongated structures in disk galaxies that can torque and funnel gas inward, influencing galaxy evolution. While strong bars are known to induce rapid inflow, the…

astro-ph.GA2025

Timescales for the Effects of Interactions on Galaxy Properties and SMBH Growth

D. O'Ryan, B. D. Simmons, A. L. Faisst +15

Galaxy interaction and merging have clear effects on the systems involved. We find an increase in the star formation rate (SFR), potential ignition of active galactic nuclei (AGN)…

astro-ph.GA20256 cited

Galaxy Zoo JWST: Up to 75% of discs are featureless at

R. J. Smethurst, B. D. Simmons, T. Géron +21

We have not yet observed the epoch at which disc galaxies emerge in the Universe. While high- measurements of large-scale features such as bars and spiral arms trace the evoluti…

astro-ph.GA2024

Structural Decomposition of Merger-Free Galaxies Hosting Luminous AGNs

Matthew J. Fahey, Izzy. L. Garland, Brooke. D. Simmons +10

Active galactic nucleus (AGN) growth in disk-dominated, merger-free galaxies is poorly understood, largely due to the difficulty in disentangling the AGN emission from that of the…