Intracluster light in clusters of galaxies at redshifts 0.4 < z < 0.8

Context. The study of intracluster light (ICL) can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, most searches and detailed studies of...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2012-01, Vol.537, p.A64
Hauptverfasser:	Guennou, L., Adami, C., Da Rocha, C., Durret, F., Ulmer, M. P., Allam, S., Basa, S., Benoist, C., Biviano, A., Clowe, D., Gavazzi, R., Halliday, C., Ilbert, O., Johnston, D., Just, D., Kron, R., Kubo, J. M., Le Brun, V., Marshall, P., Mazure, A., Murphy, K. J., Pereira, D. N. E., Rabaça, C. R., Rostagni, F., Rudnick, G., Russeil, D., Schrabback, T., Slezak, E., Tucker, D., Zaritsky, D.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology galaxies: clusters: general galaxies: clusters: intracluster medium
Online-Zugang:	Volltext
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Zusammenfassung:	Context. The study of intracluster light (ICL) can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, most searches and detailed studies of ICL have been limited to redshifts z
ISSN:	0004-6361 1432-0746 1432-0756
DOI:	10.1051/0004-6361/201117482