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Do group dynamics play a role in the evolution of member galaxies?

Hou, A. and Parker, L.C. and Balogh, M.L. and McGee, S.L. and Wilman, D.J. and Connelly, J.L. and Harris, W.E. and Mok, A. and Mulchaey, J.S. and Bower, R.G. and Finoguenov, A. (2013) 'Do group dynamics play a role in the evolution of member galaxies?', Monthly notices of Royal Astronomical Society., 435 (2). pp. 1715-1726.

Abstract

We examine galaxy groups from the present epoch to z ∼ 1 to explore the impact of group dynamics on galaxy evolution. We use group catalogues from the Sloan Digital Sky Survey (SDSS), the Group Environment and Evolution Collaboration (GEEC) and the high-redshift GEEC2 samples to study how the observed member properties depend on the galaxy stellar mass, group dynamical mass and dynamical state of the host group. We find a strong correlation between the fraction of non-star-forming (quiescent) galaxies and galaxy stellar mass, but do not detect a significant difference in the quiescent fraction with group dynamical mass, within our sample halo mass range of ∼1013–1014.5 M⊙, or with dynamical state. However, at z ∼ 0.4 we do find some evidence that the quiescent fraction in low-mass galaxies [log10(Mstar/M⊙) ≲ 10.5] is lower in groups with substructure. Additionally, our results show that the fraction of groups with non-Gaussian velocity distributions increases with redshift to z ∼ 0.4, while the amount of detected substructure remains constant to z ∼ 1. Based on these results, we conclude that for massive galaxies [log10(Mstar/M⊙) ≳ 10.5], evolution is most strongly correlated to the stellar mass of a galaxy with little or no additional effect related to either the group dynamical mass or the dynamical state. For low-mass galaxies, we do find some evidence of a correlation between the quiescent fraction and the amount of detected substructure, highlighting the need to probe further down the stellar mass function to elucidate the role of environment in galaxy evolution.

Item Type:Article
Keywords:Galaxies: formation, Galaxies: groups: general, Galaxies: kinematics and dynamics.
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Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1093/mnras/stt1410
Publisher statement:This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Record Created:07 Oct 2014 16:05
Last Modified:15 Oct 2014 16:45

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