Journal Article

The fossil phase in the life of a galaxy group

Alexander M. Von Benda-Beckmann, Elena D'Onghia, Stefan Gottlöber, Matthias Hoeft, Arman Khalatyan, Anatoly Klypin and Volker Müller

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 386, issue 4, pages 2345-2352
Published in print June 2008 | ISSN: 0035-8711
Published online April 2008 | e-ISSN: 1365-2966 | DOI:
The fossil phase in the life of a galaxy group

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We investigate the origin and evolution of fossil groups in a concordance ΛCDM cosmological simulation. We consider haloes with masses between 1 × 1013 and 5 × 1013h−1M, and study the physical mechanisms that lead to the formation of the large gap in magnitude between the brightest and the second most bright group member, which is typical for these fossil systems. Fossil groups are found to have high dark matter concentrations, which we can relate to their early formation time. The large magnitude gaps arise after the groups have built up half of their final mass, due to merging of massive group members. We show that the existence of fossil systems is primarily driven by the relatively early infall of massive satellites, and that we do not find a strong environmental dependence for these systems. In addition, we find tentative evidence for fossil group satellites falling in on orbits with typically lower angular momentum, which might lead to a more efficient merger on to the host. We find a population of groups at higher redshifts that go through a ‘fossil phase’: a stage where they show a large magnitude gap, which is terminated by renewed infall from their environment.

Keywords: methods: N-body simulations; galaxies: clusters: general; galaxies: evolution; galaxies: formation; dark matter

Journal Article.  6045 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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