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

Astronomy and Astrophysics – Astrophysics

Scientific paper

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6 pages, 4 postscript figures, accepted for publication in `Astronomy and Astrophysics'

Scientific paper

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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