{ "id": "0712.0496", "version": "v1", "published": "2007-12-04T12:07:55.000Z", "updated": "2007-12-04T12:07:55.000Z", "title": "Near-infrared evolution of brightest cluster galaxies in the most X-ray luminous clusters since z=1", "authors": [ "J. P. Stott", "A. C. Edge", "G. P. Smith", "A. M. Swinbank", "H. Ebeling" ], "comment": "9 figures, MNRAS in press", "journal": "MNRAS, Volume 384, Issue 4, pp. 1502-1510 (2008)", "doi": "10.1111/j.1365-2966.2007.12807.x", "categories": [ "astro-ph" ], "abstract": "We investigate the near infrared evolution of brightest cluster galaxies (BCGs) from a sample of rich galaxy clusters since z=1. By employing an X-ray selection of Lx>1e44 erg s-1 we limit environmental effects by selecting BCGs in comparably high density regions. We find a positive relationship between X-ray and near-infrared luminosity for BCGs in clusters with Lx>5e44 erg s-1. Applying a correction for this relation we reduce the scatter in the BCG absolute magnitude by a factor of 30%. The near-infrared J-K colour evolution demonstrates that the stellar population in BCGs has been in place since at least z=2 and that we expect a shorter period of star formation than that predicted by current hierarchical merger models. We also confirm that there is a relationship between `blue' J-K colour and the presence of BCG emission lines associated with star formation in cooling flows.", "revisions": [ { "version": "v1", "updated": "2007-12-04T12:07:55.000Z" } ], "analyses": { "keywords": [ "brightest cluster galaxies", "x-ray luminous clusters", "near-infrared evolution", "near-infrared j-k colour evolution demonstrates", "star formation" ], "tags": [ "journal article" ], "publication": { "publisher": "Wiley-Blackwell", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2008, "month": "Mar", "volume": 384, "number": 4, "pages": 1502 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 769511, "adsabs": "2008MNRAS.384.1502S" } } }