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Fig. 14.

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Stellar mass distributions for EFIGI ellipticals (E and cD galaxies noted as E) and lenticulars (S0, S0+ and S0 galaxies noted as S0) with Incl-Elong ≤ 2 in the Red Sequence. Ellipticals dominate the high-mass end of the Red Sequence, where log(M*/M) > 11.5, and lenticulars dominate the lower-mass part.

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