Home > Research > Publications & Outputs > The behaviour of dark matter associated with fo...

Electronic data

  • 1504.03388

    Accepted author manuscript, 4.04 MB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

Links

Text available via DOI:

View graph of relations

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

Research output: Contribution to journalJournal articlepeer-review

Published
  • Richard Massey
  • Liliya Williams
  • Renske Smit
  • Mark Swinbank
  • Thomas D. Kitching
  • David Harvey
  • Mathilde Jauzac
  • Holger Israel
  • Douglas Clowe
  • Alastair Edge
  • Matt Hilton
  • Eric Jullo
  • Adrienne Leonard
  • Jori Liesenborgs
  • Julian Merten
  • Irshad Mohammed
  • Daisuke Nagai
  • Johan Richard
  • Andrew Robertson
  • Prasenjit Saha
  • Rebecca Santana
  • Eric Tittley
Close
<mark>Journal publication date</mark>1/06/2015
<mark>Journal</mark>Monthly Notices of the Royal Astronomical Society
Issue number4
Volume449
Number of pages14
Pages (from-to)3393-3406
Publication StatusPublished
Early online date9/04/15
<mark>Original language</mark>English

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(-0.49)(+0.47) 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 sigma(DM)/(m) similar to (1.7 +/- 0.7) x 10(-4) cm(2) g(-1) x (t(infall)/10(9) yr)(-2), where t(infall) is the infall duration.