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Title:
Galaxies in most dense environments at redshift 1.4
Authors:
Strazzullo, V.
Affiliation:
AA(Irfu/SAp, CEA-Saclay, Orme des Merisiers, 91191 Gif sur Yvette, France )
Publication:
The Intriguing Life of Massive Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 295, pp. 61-61
Publication Date:
07/2013
Origin:
CUP
Keywords:
Galaxies: clusters, Galaxies: evolution, Galaxies: high-redshift,
Abstract Copyright:
(c) 2013: Copyright © International Astronomical Union 2013
DOI:
10.1017/S1743921313004316
Bibliographic Code:
2013IAUS..295...61S

Abstract

At a cosmic time when galaxy clusters start showing evidence of a still active galaxy population, the X-ray luminous, massive cluster XMMU J2235-2557 at z=1.39, already hosts massive, quiescent, early-type galaxies on a tight red sequence dominating the cluster core. XMMU J2235-2557 is among the most massive of the very distant clusters, which may explain the evolved status of the system itself, and of its host galaxy populations. It remains a unique laboratory to observe environment-biased galaxy evolution already 9 billion years ago.

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