J.T.C.G. Head
Dissecting the red sequence: the bulge and disc colours of early-type galaxies in the Coma cluster
Head, J.T.C.G.; Lucey, J.R.; Hudson, M.J.; Smith, R.J.
Authors
John Lucey john.lucey@durham.ac.uk
Emeritus Professor
M.J. Hudson
Dr Russell Smith russell.smith@durham.ac.uk
Assistant Professor
Abstract
We explore the internal structure of red-sequence galaxies in the Coma cluster across a wide range of luminosities (−17 > Mg > −22) and cluster-centric radii (0 < rcluster < 1.3 r200). We present the 2D bulge-disc decomposition of galaxies in deep Canada–France–Hawaii Telescope u, g, i imaging using GALFIT. Rigorous filtering is applied to identify an analysis sample of 200 galaxies which are well described by an ‘archetypal’ S0 structure (central bulge + outer disc). We consider internal bulge and/or disc colour gradients by allowing component sizes to vary between bands. Gradients are required for 30 per cent of analysis sample galaxies. Bulge half-light radii are found to be uncorrelated with galaxy luminosity (Re ∼ 1 kpc, n ∼ 2) for all but the brightest galaxies (Mg < −20.5). The S0 discs are brighter (at fixed size, or smaller at fixed luminosity) than those of star-forming spirals. A similar colour–magnitude relation is found for both bulges and discs. The global red sequence for S0s in Coma hence results from a combination of both component trends. We measure an average bulge – disc colour difference of 0.09 ± 0.01 mag in g − i, and 0.16 ± 0.01 mag in u − g. Using simple stellar population models, bulges are either ∼2–3 times older, or ∼ 2 times more metal rich than discs. The trend towards bluer global S0 colours observed further from Coma's core is driven by a significant correlation in disc colour with cluster-centric radius. An equivalent trend is detected in bulge colours at a marginal significance level. Our results therefore favour environment-mediated mechanisms of disc fading as the dominant factor in S0 formation.
Citation
Head, J., Lucey, J., Hudson, M., & Smith, R. (2014). Dissecting the red sequence: the bulge and disc colours of early-type galaxies in the Coma cluster. Monthly Notices of the Royal Astronomical Society, 440(2), 1690-1711. https://doi.org/10.1093/mnras/stu325
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 14, 2014 |
Online Publication Date | Mar 26, 2014 |
Publication Date | May 11, 2014 |
Deposit Date | Apr 4, 2014 |
Publicly Available Date | Apr 7, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 440 |
Issue | 2 |
Pages | 1690-1711 |
DOI | https://doi.org/10.1093/mnras/stu325 |
Keywords | Galaxies, Clusters, Abell 1656, Elliptical and lenticular, CD, Evolution, Formation, Structure. |
Public URL | https://durham-repository.worktribe.com/output/1467135 |
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Copyright Statement
Advance online version This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Authors
Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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