@Article{Hansen_etal2000,
author="Hansen, Lene
and J{\o}rgensen, H. E.
and N{\o}rgaard-Nielsen, Hans Ulrik
and Pedersen, Kenneth
and Goudfrooij, P.
and Linden-Vornle, M. J. D.",
title="ISO far-infrared observations of rich galaxy clusters III. Abell 2029, Abell 2052, Abell 2142",
journal="Astron. Astrophys.",
year="2000",
volume="362",
number="1",
pages="133--137",
abstract="A sample of five rich galaxy clusters has been mapped by ISO at 60 $\mu$m, 100 $\mu$m, 135 $\mu$m, and 200 $\mu$m using the PHT-C camera. In previous papers Abell 2670 and Sersic 159-03 were discussed. Here we present the results for Abell 2029, Abell 2052, and Abell 2142. The conclusion of the survey is that the relatively small fields (approximate to 60 square are minutes) are structured with filaments or superpositions of point sources. In some cases point sources (approximate to 0.1 Jy) can be identified with cluster galaxies. An attempt to demonstrate infrared emission from dust in the cooling flows (due to star formation) was inconclusive.",
optnote="exported from refbase (https://db.rplab.ru/refbase/show.php?record=456), last updated on Sat, 04 Jun 2016 09:40:39 -0500"
}