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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
Affiliation:
ESO, Alonso de Cordova 3107, Vitacura, Santiago de Chile, Chile email: [email protected]
C. Adami
Affiliation:
Aix Marseille Université, CNRS, LAM, UMR 7326, F-13388 Marseille, France email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

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