ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03
| dc.creator | Hansen, L. | |
| dc.creator | Jorgensen, H. E. | |
| dc.creator | Norgaard-Nielsen, H. U. | |
| dc.creator | Pedersen, K. | |
| dc.creator | Goudfrooij, P. | |
| dc.creator | Linden-Vornle, M. J. D. | |
| dc.date | 2000-02-22 | |
| dc.date.accessioned | 2026-07-07T01:52:25Z | |
| dc.date.available | 2026-07-07T01:52:25Z | |
| dc.description | 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. | |
| dc.description | 6 pages, 4 postscript figures, accepted for publication in `Astronomy and Astrophysics' | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0002403 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0002403 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/615 | |
| dc.subject | Astrophysics | |
| dc.title | ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03 | |
| dc.type | text |