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Journal article

ISO far-infrared observations of rich galaxy clusters I. Abell 2670

By Hansen, Lene1; Jorgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik2,3; Pedersen, Kenneth4,5; Goudfrooij, P.; Linden-Vornle, M.J.D.

From

National Food Institute, Technical University of Denmark1

Astrophysics, National Space Institute, Technical University of Denmark2

National Space Institute, Technical University of Denmark3

Electric Power Engineering, Department of Electrical Engineering, Technical University of Denmark4

Department of Electrical Engineering, Technical University of Denmark5

As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals at the cluster distance.

Probable optical counterparts are cluster galaxies with various characteristics such as blue colour, Ha emission, or double nuclei. One source is extended which could possibly be emission from intracluster dust in debris from spiral galaxies.

Language: English
Year: 1999
Pages: 406-410
ISSN: 14320746 and 00046361
Types: Journal article
ORCIDs: Nørgaard-Nielsen, Hans Ulrik
Keywords

galaxies : clusters : individual : Abell 2670 infrared : galaxies

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