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IPM
30
YEARS OLD

“School of Astronomy”

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Paper   IPM / Astronomy / 13418
School of Astronomy
  Title:   Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
  Author(s): 
1.  M. Raouf
2.  H. G.Khosroshahi
3.  T. Ponman
4.  A Dariush
5.  A. Molaeinezhad
6.  S. Tavasoli
  Status:   Published
  Journal: MNRAS
  Vol.:  442
  Year:  2014
  Pages:   10
  Supported by:            IPM IPM
  Abstract:
There have been a number of studies dedicated to identification of fossil galaxy groups, arguably groups with a relatively old formation epoch. Most of such studies identify fossil groups, primarily based on a large luminosity gap, which is the magnitude gap between the two most luminous galaxies in the group. Studies of these types of groups in the millennium cosmological simulations show that, although they have accumulated a significant fraction of their mass, relatively earlier than groups with a small luminosity gap, this parameter alone is not highly efficient in fully discriminating between the öld" and ÿoung" galaxy groups, a label assigned based on halo mass accumulation history. We study galaxies drawn from the semi-analytic models of Guo et al. (2011), based on the Millennium Simulation. We establish a set of four observationally measurable parameters which can be used in combination, to identify a subset of galaxy groups which are old, with a very high probability. We thus argue that a sample of fossil groups selected based on luminosity gap will result in a contaminated sample of old galaxy groups. By adding constraints on the luminosity of the brightest galaxy, and its offset from the group luminosity centroid, we can considerably improve the age-dating.

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