A1 Refereed original research article in a scientific journal

Galaxy and Mass Assembly (GAMA): variation in galaxy structure across the green valley




AuthorsKelvin LS, Bremer MN, Phillipps S, James PA, Davies LJM, De Propris R, Moffett AJ, Percival SM, Baldry IK, Collins CA, Alpaslan M, Bland-Hawthorn J, Brough S, Cluver M, Driver SP, Hashemizadeh A, Holwerda BW, Laine J, Lara-Lopez MA, Liske J, Maciejewski W, Napolitano NR, Penny SJ, Popescu CC, Sansom AE, Sutherland W, Taylor EN, Kampen E, Wang L

PublisherOXFORD UNIV PRESS

Publication year2018

JournalMonthly Notices of the Royal Astronomical Society

Journal name in sourceMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Journal acronymMON NOT R ASTRON SOC

Volume477

Issue3

First page 4116

Last page4130

Number of pages15

ISSN0035-8711

eISSN1365-2966

DOIhttps://doi.org/10.1093/mnras/sty933

Web address https://academic.oup.com/mnras/article/477/3/4116/4970787#116726248


Abstract
Using a sample of 472 local Universe (z < 0.06) galaxies in the stellar mass range 10.25 < logM(star)/M-circle dot < 10.75, we explore the variation in galaxy structure as a function of morphology and galaxy colour. Our sample of galaxies is subdivided into red, green, and blue colour groups and into elliptical and non-elliptical (disk-type) morphologies. Using Kilo-Degree Survey (KiDS) and Visible and Infrared Survey Telescope for Astronomy (VISTA) Kilo-Degree Infrared Galaxy Survey (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 (2.3 sigma) and lenses (2.9 sigma) in disk-type galaxies as they transition across the green valley. Combined, this implies a joint ring/lens green valley surplus significance of 3.3 sigma relative to equivalent disk-types within either the blue cloud or the red sequence. We recover a bar fraction of similar to 44 per cent which remains flat with colour, however, we find that the presence of a bar acts to modulate the incidence of rings and (to a lesser extent) lenses, with rings in barred disk-type galaxies more common by similar to 20-30 percentage points relative to their unbarred counterparts, regardless of colour. Additionally, green valley disk-type galaxies with a bar exhibit a significant 3.0 sigma surplus of lenses relative to their blue/red analogues. The existence of such structures rules out violent transformative events as the primary end-of-life evolutionary mechanism, with a more passive scenario the favoured candidate for the majority of galaxies rapidly transitioning across the green valley.



Last updated on 2024-26-11 at 23:53