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ICL light in a z~0.5 cluster: the MUSE perspective

Published online by Cambridge University Press:  21 March 2017

E. Pompei ,
C. Adami  and
the XXL team
E. Pompei
Affiliation:
ESO, Alonso de Cordova 3107, Vitacura, Santiago de Chile, Chile email: epompei@eso.org
C. Adami
Affiliation:
Aix Marseille Université, CNRS, LAM, UMR 7326, F-13388 Marseille, France email: christophe.adami@lam.fr
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Abstract

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Intracluster light is contributed by both stars and gas and it is an important tracer of the interaction history of galaxies within a cluster. We present here the results obtained from MUSE observations of an intermediate redshift (z~ 0.5) cluster taken from the XXL survey and we conclude that the most plausible process responsible for the observed amount of ICL is ram pressure stripping.

Keywords

galaxiesclustersintracluster light3D spectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 336 - 338
Copyright
Copyright © International Astronomical Union 2017 

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