Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827.

Massey, R. and Williams, L. and Smit, R. and Swinbank, M. and Kitching, D. and Harvey, D. and Jauzac, M. and Israel, H. and Clowe, D. and Edge, A. and Hilton, M. and Jullo, E. and Leonard, A. and Liesenborgs, J. and Merten, J. and Mohammed, I. and Nagai, D. and Richard, J. and Robertson, A. and Saha, P. and Santana, R. and Stott, J. and Tittley, E. (2015) 'The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827.', Monthly notices of the Royal Astronomical Society., 449 (4). pp. 3393-3406.

Abstract

Galaxy cluster Abell 3827 hosts the stellar remnants of four almost equally bright elliptical galaxies within a core of radius 10 kpc. Such corrugation of the stellar distribution is very rare, and suggests recent formation by several simultaneous mergers. We map the distribution of associated dark matter, using new Hubble Space Telescope imaging and Very Large Telescope/Multi-Unit Spectroscopic Explorer integral field spectroscopy of a gravitationally lensed system threaded through the cluster core. We find that each of the central galaxies retains a dark matter halo, but that (at least) one of these is spatially offset from its stars. The best-constrained offset is 1.62+0.47−0.49 kpc, where the 68 per cent confidence limit includes both statistical error and systematic biases in mass modelling. Such offsets are not seen in field galaxies, but are predicted during the long infall to a cluster, if dark matter self-interactions generate an extra drag force. With such a small physical separation, it is difficult to definitively rule out astrophysical effects operating exclusively in dense cluster core environments – but if interpreted solely as evidence for self-interacting dark matter, this offset implies a cross-section σDM/m ∼ (1.7 ± 0.7) × 10−4 cm2 g−1 × (tinfall/109 yr)−2, where tinfall is the infall duration.

Item Type:Article
Keywords:Astroparticle physics, Gravitational lensing, Strong galaxies, Clusters: individual, Abell 3827, Dark matter
Full text:PDF - Published Version (5186Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1093/mnras/stv467
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Record Created:14 Apr 2015 19:20
Last Modified:01 Jun 2015 09:29

Social bookmarking: del.icio.usConnoteaBibSonomyCiteULikeFacebookTwitterExport: EndNote, Zotero | BibTex
Usage statisticsLook up in GoogleScholar | Find in a UK Library