ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03
  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. 
L. Hansen, H.E. Jorgensen, H.U. Norgaard-Nielsen, K. Pedersen, P.   Goudfrooij, M.J.D. Linden-Vornle