Are fossil groups a challenge of the Cold Dark Matter paradigm?
Stefano Zibetti (1), Daniele Pierini (2), Gabriel W. Pratt (2) ((1), MPIA Heidelberg, Germany, (2) MPE Garching, Germany)

TL;DR
This study investigates fossil galaxy groups to determine if they challenge the Cold Dark Matter paradigm, finding their properties align with normal clusters and do not lack substructure as previously thought.
Contribution
The paper confirms the fossil nature of several galaxy systems and shows their substructure distribution functions are consistent with standard cosmological models.
Findings
Fossil systems have luminosity functions similar to universal cluster functions.
CSDFs of fossil systems match those of normal clusters and simulations.
Contrary to earlier claims, fossil groups do not lack substructure.
Abstract
We study six groups and clusters of galaxies suggested in the literature to be `fossil' systems (i.e. to have luminous diffuse X-ray emission and a magnitude gap of at least 2 mag-R between the first and the second ranked member within half of the virial radius), each having good quality X-ray data and SDSS spectroscopic or photometric coverage out to the virial radius. The poor cluster AWM4 is clearly established as a fossil system, and we confirm the fossil nature of four other systems (RXJ1331.5+1108, RXJ1340.6+4018, RXJ1256.0+2556 and RXJ1416.4+2315), while the cluster RXJ1552.2+2013 is disqualified as fossil system. For all systems we present the luminosity functions within 0.5 and 1 virial radius that are consistent, within the uncertainties, with the universal luminosity function of clusters. For the five bona fide fossil systems, having a mass range 2x10^13-3x10^14 M_Sun, we…
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