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2000A&A...362..133H - Astronomy and Astrophysics, volume 362133-137 (2000/10-1)
ISO far-infrared observations of rich galaxy clusters. III. Abell 2029, Abell 2052, Abell 2142.
HANSEN L., JORGENSEN H.E., NORGAARD-NIELSEN H.U., PEDERSEN K., GOUDFROOIJ P. and LINDEN-VORNLE M.J.D.
Abstract (from CDS):
A sample of five rich galaxy clusters has been mapped by ISO at 60µm, 100µm, 135µm, and 200µm 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 (≃60 square arc minutes) are structured with filaments or superpositions of point sources. In some cases point sources (≃0.1Jy) can be identified with cluster galaxies. An attempt to demonstrate infrared emission from dust in the cooling flows (due to star formation) was inconclusive.
Abstract Copyright: ∼
Journal keyword(s): galaxies: clusters: individual: Abell 2029, Abell 2052, Abell 2142 - infrared: galaxies
Nomenclature: Fig.3, Table 3: [HJN2000b] ACO 2052 N (Nos 1-4).
Simbad objects: 5
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