No CrossRef data available.
Article contents
ICL light in a z~0.5 cluster: the MUSE perspective
Published online by Cambridge University Press: 21 March 2017
Abstract
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