activity
20242026
collaborators

12 papers

astro-ph.GA2026

Spiral Morphology and Radial Migration: Kinematically heating, cooling, and cold

Kathryne J. Daniel, M. E. Wisz, Karen L. Masters +3

Transient spiral arms are known to drive radial redistribution of stars and thus could play a central role in shaping disk galaxies, including modifying, over time, the age, chemic…

astro-ph.GA2026

Deep Learning Segmentation of Spiral Arms and Bars for 600,000 Galaxies in DESI

Ashley Spindler, Mike Walmsley, Karen L. Masters +4

We present a catalogue of segmentation maps identifying the extent of spiral arms and bars of 639,636 galaxies in the DESI Legacy Survey. To produce these maps, we have trained a d…

astro-ph.GA2026

Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1

Tenley Hutchinson-Smith, Brooke D. Simmons, Karen L. Masters +12

Understanding the role of galactic scale bars in disk galaxy evolution requires detailed measurements of bar properties across galaxies hosting bars at many redshifts. We present m…

astro-ph.GA2026

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

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.GA2025

The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies

M. E. Wisz, Karen L. Masters, Kathryne J. Daniel +2

As galaxies evolve over time, the orbits of their constituent stars are expected to change in size and shape, moving stars away from their birth radius. Radial gas flows are also e…