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The elliptical galaxy colour-magnitude relation as a discriminant between the monolithic and merger paradigms

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Academic year: 2021

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Figure

Figure 1. The model colour–magnitude relation at z = 0. Top: CMR se- se-quence with a linear least-squares fit (dotted line) and a progressive  one-sigma fit to the sample
Figure 2. Intracluster scatter as a fraction of the total scatter plotted against the elliptical occupancy of each cluster.
Figure 4. Age–metallicity parameter space in model cluster ellipticals split into luminosity classes
Figure 7. Redshift evolution of the slope and scatter in the model (U − V ) versus V CMR
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