Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-08-28
Mon.Not.Roy.Astron.Soc.372:1856-1868,2006
Astronomy and Astrophysics
Astrophysics
15 pages, 5 figures. Accepted for publication in MNRAS. Corrected F&S numbers for NGC1400 group and typos in references list
Scientific paper
10.1111/j.1365-2966.2006.10993.x
We have redefined group membership of six southern galaxy groups in the local universe (mean cz < 2000 km/s) based on new redshift measurements from our recently acquired Anglo-Australian Telescope 2dF spectra. For each group, we investigate member galaxy kinematics, substructure, luminosity functions and luminosity-weighted dynamics. Our calculations confirm that the group sizes, virial masses and luminosities cover the range expected for galaxy groups, except that the luminosity of NGC 4038 is boosted by the central starburst merger pair. We find that a combination of kinematical, substructural and dynamical techniques can reliably distinguish loose, unvirialised groups from compact, dynamically relaxed groups. Applying these techniques, we find that Dorado, NGC 4038 and NGC 4697 are unvirialised, whereas NGC 681, NGC 1400 and NGC 5084 are dynamically relaxed.
Drinkwater Michael. J.
Evstigneeva Ekaterina
Firth P.
Gregg Michael D.
Jones Jeremy B.
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