Fig. 17.

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M*/MDM as a function of stellar mass for central disc and lenticular galaxies at z = 1 and z = 0. The colour scheme corresponds to the mean number of major mergers for each bin since z = 2. The top left panel represents the disc descendants that do not develop a bar, whereas the top right panel represents those that develop a bar. The bottom row corresponds to those galaxies at redshift z = 1. Lenticular and disc galaxies that form a bar after z = 1 experience more mergers and have higher stellar-to-dark matter ratios than those galaxies that never form a bar for a given stellar mass.
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