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ICL light in a z~0.5 cluster: the MUSE perspective
Published online by Cambridge University Press: 21 March 2017
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
- 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
References
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Pierre, M., Pacaud, F., Adami, C., Alis, S., Altieri, B.
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2015, A&A accepted 2015, XXL Paper IGoogle Scholar
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