William S. Burgett
Substructure analysis of selected low-richness 2dFGRS clusters of galaxies
Burgett, William S.; Vick, Michael M.; Davis, David S.; Colless, Matthew; De Propris, Roberto; Baldry, Ivan; Baugh, Carlton; Bland-Hawthorn, Joss; Bridges, Terry; Cannon, Russell; Cole, Shaun; Collins, Chris; Couch, Warrick; Cross, Nicholas; Dalton, Gavin; Driver, Simon; Efstathiou, George; Ellis, Richard; Frenk, Carlos S.; Glazebrook, Karl; Hawkins, Edward; Jackson, Carole; Lahav, Ofer; Lewis, Ian; Lumsden, Stuart; Maddox, Steve; Madgwick, Darren; Norberg, Peder; Peacock, John A.; Percival, Will; Peterson, Bruce; Sutherland, Will; Taylor, Keith
Authors
Michael M. Vick
David S. Davis
Matthew Colless
Roberto De Propris
Ivan Baldry
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
Joss Bland-Hawthorn
Terry Bridges
Russell Cannon
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Chris Collins
Warrick Couch
Nicholas Cross
Gavin Dalton
Simon Driver
George Efstathiou
Richard Ellis
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Karl Glazebrook
Edward Hawkins
Carole Jackson
Ofer Lahav
Ian Lewis
Stuart Lumsden
Steve Maddox
Darren Madgwick
Professor Peder Norberg peder.norberg@durham.ac.uk
Professor
John A. Peacock
Will Percival
Bruce Peterson
Will Sutherland
Keith Taylor
Abstract
Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in clusters of galaxies are applied to recently obtained data from the 2dF Galaxy Redshift Survey. The sample of 25 clusters used in this study includes 16 clusters not previously investigated for substructure. Substructure is detected at or greater than the 99 per cent confidence level in at least one test for 21 of the 25 clusters studied here. From the results, it appears that low-richness clusters commonly contain subclusters participating in mergers. About half of the clusters have two or more components within 0.5 h−1 Mpc of the cluster centroid, and at least three clusters (Abell 1139, Abell 1663 and Abell S333) exhibit velocity–position characteristics consistent with the presence of possible cluster rotation, shear, or infall dynamics. The geometry of certain features is consistent with influence by the host supercluster environments. In general, our results support the hypothesis that low-richness clusters relax to structureless equilibrium states on very long dynamical time-scales (if at all).
Citation
Burgett, W. S., Vick, M. M., Davis, D. S., Colless, M., De Propris, R., Baldry, I., …Taylor, K. (2004). Substructure analysis of selected low-richness 2dFGRS clusters of galaxies. Monthly Notices of the Royal Astronomical Society, 352(2), 605-654. https://doi.org/10.1111/j.1365-2966.2004.07952.x
Journal Article Type | Article |
---|---|
Publication Date | 2004-08 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 352 |
Issue | 2 |
Pages | 605-654 |
DOI | https://doi.org/10.1111/j.1365-2966.2004.07952.x |
Public URL | https://durham-repository.worktribe.com/output/1615648 |
Related Public URLs | http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004MNRAS.352..605B&db_key=AST |
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