Medium-distant clusters of galaxies seen by ISO

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dc.creatorLemonon, L.
dc.creatorPierre, M.
dc.creatorCesarsky, C. J.
dc.creatorElbaz, D.
dc.creatorVigroux, L.
dc.date1998-11-30
dc.date.accessioned2026-07-07T02:29:22Z
dc.date.available2026-07-07T02:29:22Z
dc.descriptionWe present a comprehensive study of ISO cluster galaxies in connection with other wavelengths. First results show that infrared galaxies detected by ISOCAM concentrate on the edge of clusters. Surprisingly, they are not emission lines galaxies but very luminous elliptical, merging or interacting ones, which suggests non-trivial connections between star formation rate, optical and mid-IR properties. However, no correlation has been found between the MIR/optical star formation properties of the galaxies, so that the exact origin of the IR emission remains unclear.
dc.description4 pages, 3 figures, to appear in 'The Universe as seen by ISO', eds. P. Cox and M.F. Kessler
dc.identifierhttps://arxiv.org/abs/astro-ph/9811467
dc.identifierhttp://arxiv.org/abs/astro-ph/9811467
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13443
dc.subjectAstrophysics
dc.titleMedium-distant clusters of galaxies seen by ISO
dc.typetext

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