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ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03

L. Hansen·H. E. Jorgensen·H. U. Norgaard-Nielsen·K. Pedersen·P. Goudfrooij·M. J. D. Linden-Vornle
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Abstract

The far-infrared emission from rich galaxy clusters is investigated. Maps have been obtained by ISO at 60, 100, 135, and 200 microns using the PHT-C camera. Ground based imaging and spectroscopy were also acquired. Here we present the results for the cooling flow cluster Sersic 159-03. An infrared source coincident with the dominant cD galaxy is found. Some off-center sources are also present, but without any obvious counterparts.

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L. Hansen, H. E. Jorgensen, H. U. Norgaard-Nielsen, K. Pedersen, P. Goudfrooij, M. J. D. Linden-Vornle. 2000-02-22. ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03. https://arxiv.org/abs/astro-ph/0002403

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