Colours of Bulges and Discs within Galaxy Clusters and the Signature of Disc Fading on Infall
Michael J. Hudson, Jeffrey B. Stevenson, Russell J. Smith, Gary A., Wegner, John R. Lucey, Luc Simard

TL;DR
This study investigates the colours of bulges and discs in cluster galaxies, revealing that bulge colours are mainly mass-dependent while disc colours are influenced by environment, indicating different galaxy evolution processes.
Contribution
It provides a detailed analysis of bulge and disc colours in a large galaxy sample, highlighting the environmental impact on disc colours and the dominance of bulge properties in the colour-magnitude relation.
Findings
Bulge colours follow a strong colour-magnitude relation.
Disc colours are bluer than bulges by 0.24 magnitudes.
Discs in cluster centers are redder than those at the virial radius.
Abstract
The origins of the bulge and disc components of galaxies are of primary importance to understanding galaxy formation. Here bulge-disc decomposition is performed simultaneously in B- and R-bands for 922 bright galaxies in 8 nearby (z < 0.06) clusters with deep redshift coverage using photometry from the NOAO Fundamental Plane Survey. The total galaxy colours follow a universal colour-magnitude relation (CMR). The discs of L_* galaxies are 0.24 magnitudes bluer in than bulges. Bulges have a significant CMR slope while the CMR slope of discs is flat. Thus the slope of the CMR of the total light is driven primarily (60%) by the bulge-CMR, and to a lesser extent (40%) by the change in the bulge-to-total ratio as a function of magnitude. The colours of the bulge and disc components do not depend on the bulge-to-total ratio, for galaxies with bulge-to-total ratios greater than 0.2. While…
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