Galaxy and Mass Assembly (GAMA): Variation in Galaxy Structure Across the Green Valley
Lee S. Kelvin, Malcolm N. Bremer, Steven Phillipps, Philip A. James,, Luke J. M. Davies, Roberto De Propris, Amanda J. Moffett, Susan M. Percival,, Ivan K. Baldry, Chris A. Collins, Mehmet Alpaslan, Joss Bland-Hawthorn, Sarah, Brough, Michelle Cluver, Simon P. Driver

TL;DR
This study investigates how galaxy structures like rings, lenses, and bars vary across the green valley in the local universe, revealing insights into galaxy evolution and the passive transition process.
Contribution
It provides new evidence of increased rings and lenses in disk galaxies crossing the green valley and examines the role of bars in galaxy structural features.
Findings
Surplus of rings and lenses in green valley disk galaxies
Bar presence correlates with higher incidence of rings and lenses
Passive evolution likely dominates galaxy transition across the green valley
Abstract
Using a sample of 472 local Universe (z<0.06) galaxies in the stellar mass range 10.25 < log M*/M_sun < 10.75, we explore the variation in galaxy structure as a function of morphology and galaxy colour. Our sample of galaxies is sub-divided into red, green and blue colour groups and into elliptical and non-elliptical (disk-type) morphologies. Using KiDS and VIKING derived postage stamp images, a group of eight volunteers visually classified bars, rings, morphological lenses, tidal streams, shells and signs of merger activity for all systems. We find a significant surplus of rings () and lenses () in disk-type galaxies as they transition across the green valley. Combined, this implies a joint ring/lens green valley surplus significance of relative to equivalent disk-types within either the blue cloud or the red sequence. We recover a bar fraction of ~44%…
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