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Dust in Clusters of Galaxies and the Sunyaev Zel'dovich Effect1
Published online by Cambridge University Press: 13 May 2016
Abstract
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We review here the unique opportunity provided by the sub-millimeter/millimeter domain to characterize both the warm intra-cluster plasma via the Sunyaev Zel'dovich Effect (SZE) on the cosmic microwave background, and the dust within this plasma via its thermal emission. However, multi-wavelength measurements are needed in order to separate these effects from the foreground galactic dust and the background infrared galaxies.
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- Copyright © Astronomical Society of the Pacific 2001
References
Lamarre, J. M., Giard, M., Pointecouteau, E., Bernard, J. P., Serra, G., Pajot, F., Desert, F. X., Ristorcelli, I., Torre, J. P., Church, S., Coron, N., Puget, J. L., & Bock, J. J.
1998, ApJ, 507, L5
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