We have investigated the redshift evolution of the colour-clustercentric radius relation and the morphology-clustercentric radius relation in three redshift bins, 0.02 ≤ z ≤ 0.14, 0.14 < z ≤ 0.20 and 0.20
CITATION STYLE
Goto, T., Yagi, M., Tanaka, M., & Okamura, S. (2004). Evolution of the colour-radius and morphology-radius relations in SDSS galaxy clusters. Monthly Notices of the Royal Astronomical Society, 348(2), 515–518. https://doi.org/10.1111/j.1365-2966.2004.07324.x
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