Fig. 8.
CMD of the 3C 129 cluster identified as members. Colours indicate morphological type. Circles are the red-sequence galaxies, and those enclosed in squares are H I detected galaxies within the radius and velocity range of the cluster. The dotted lines show the ±3σ rms dispersion (0.12 mag) from the fitted red sequence relation: J − K = −0.023K + 1.25.
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