Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-04-24
Mon.Not.Roy.Astron.Soc.378:1507-1530,2007
Astronomy and Astrophysics
Astrophysics
21 pages plus appendices, accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2007.11900.x
We present an examination of the kinematics and stellar populations of a sample of 3 Brightest Group Galaxies (BGGs) and 3 Brightest Cluster Galaxies (BCGs) in X-ray groups and clusters. We have obtained high signal-to-noise Gemini/GMOS (Gemini South Multi-Object Spectrograph) long-slit spectra of these galaxies and use Lick indices to determine ages, metallicities and alpha-element abundance ratios out to at least their effective radii. We find that the BGGs and BCGs have very uniform masses, central ages and central metallicities. Examining the radial dependence of their stellar populations, we find no significant velocity dispersion, age, or alpha-enhancement gradients. However, we find a wide range of metallicity gradients, suggesting a variety of formation mechanisms. The range of metallicity gradients observed is surprising given the homogeneous environment these galaxies probe and their uniform central stellar populations. However, our results are inconsistent with any single model of galaxy formation and emphasize the need for more theoretical understanding of both the origins of metallicity gradients and galaxy formation itself. We postulate two possible physical causes for the different formation mechanisms.
Brough Sarah
Burke Daniel
Collins Cami
Couch Warrick
Forbes Duncan
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