Quick Search:

uzh logo
Browse by:

Zurich Open Repository and Archive

Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-48292

Brough, S; Tran, K V; Sharp, R G; von der Linden, A; Couch, W J (2011). Spatial kinematics of brightest cluster galaxies and their close companions from integral field unit spectroscopy. Monthly Notices of the Royal Astronomical Society. Letters, 414(1):L80-L84.

Accepted Version
View at publisher


We present Integral Field Unit (IFU) spectroscopy of four brightest cluster galaxies (BCGs) at z ˜ 0.1. Three of the BCGs have close companions within a projected radius of 20 kpc and one has no companion within that radius. We calculate the dynamical masses of the BCGs and their companions to be ?. We estimate the probability that the companions of the BCGs are bound using the observed masses and velocity offsets. We show that the lowest mass companion (1:4) is not bound while the two nearly equal mass (1:1.45 and 1:1.25) companions are likely to merge with their host BCGs in 0.35 Gyr in major, dry mergers. We conclude that some BCGs continue to grow from major merging even at z ˜ 0. We analyse the stellar kinematics of these systems using the λR parameter developed by the SAURON team. This offers a new and unique means to measure the stellar angular momentum of BCGs and make a direct comparison to other early-type galaxies. The BCGs and their companions have similar ellipticities to those of other early-type galaxies but are more massive. We find that not all these massive galaxies have low ? as one might expect. One of the four BCGs and the two massive companions are found to be fast-rotating galaxies with high angular momentum, thereby providing a new test for models of galaxy evolution and the formation of intracluster light.


19 citations in Web of Science®
21 citations in Scopus®
Google Scholar™



44 downloads since deposited on 18 Feb 2012
11 downloads since 12 months

Detailed statistics

Additional indexing

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
Dewey Decimal Classification:530 Physics
Date:April 2011
Deposited On:18 Feb 2012 20:08
Last Modified:05 Apr 2016 14:55
ISSN:0035-8711 (P) 1365-2966 (E)
Additional Information:The definitive version is available at www3.interscience.wiley.com
Publisher DOI:10.1111/j.1745-3933.2011.01060.x
Related URLs:http://arxiv.org/abs/1104.1239

Users (please log in): suggest update or correction for this item

Repository Staff Only: item control page