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arXiv · 1201.5491

The radial distribution of galaxies in groups and clusters

J. M. Budzynski·S. Koposov·I. G. McCarthy·S. L. McGee·V. Belokurov
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Abstract

We present a new catalogue of 55,121 groups and clusters centred on Luminous Red Galaxies from SDSS DR7 in the redshift range 0.15 ~2.6) that is approximately a factor of two lower than that of the dark matter (as predicted by N-body cosmological simulations) and nearly independent of halo mass. Interestingly, in spite of the difference in shape between the galaxy and dark matter radial distributions, both exhibit a high degree of self-similarity. A self-consistent comparison to several recent semi-analytic models of galaxy formation indicates that: (1) beyond ~0.3 r_500 current models are able to reproduce both the shape and normalisation of the satellite profiles; and (2) within ~0.3 r_500 the predicted profiles are sensitive to the details of the satellite-BCG merger timescale calculation. The former is a direct result of the models being tuned to match the global galaxy luminosity function combined with the assumption that the satellite galaxies do not suffer significant tidal stripping, even though their surrounding dark matter haloes can be removed through this process. Combining our results with measurements of the intracluster light should provide a way to inform theoretical models on the efficacy of the tidal stripping and merging processes.

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J. M. Budzynski, S. Koposov, I. G. McCarthy, S. L. McGee, V. Belokurov. 2012-01-26. The radial distribution of galaxies in groups and clusters. https://doi.org/10.1111/j.1365-2966.2012.20663.x

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