Abstract
Parameters of the distant galaxy clusters of 3C295 (z=0.46) and Cl 0024+1654 (z=0.39) are compared with the predictions made using galaxies of the local clusters Coma (z=0.023) and DC 0329−52 (z=0.057) taking theK-effect into account. The distributions of colour and morphological type, and the amplitudesF +/F− of the λ0 4000 discontinuity are examined and no evidence for evolution of the galaxies and the clusters can be seen.
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Laurikainen, E., Jaakkola, T. On the existence of cosmological evolutionary effects. Astrophys Space Sci 109, 111–122 (1985). https://doi.org/10.1007/BF00651018
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DOI: https://doi.org/10.1007/BF00651018