Deep ISOCAM view of the core of the lensing cluster A2390

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dc.creatorLemonon, L.
dc.creatorPierre, M.
dc.creatorCesarsky, C. J.
dc.creatorElbaz, D.
dc.creatorPello, R.
dc.creatorSoucail, G.
dc.creatorVigroux, L.
dc.date1998-04-08
dc.date.accessioned2026-07-07T02:26:33Z
dc.date.available2026-07-07T02:26:33Z
dc.descriptionWe have imaged the inner square arcminute of the well known lensing and cooling flow cluster A2390 (z = 0.23) down to a sensitivity of 65 and 130 microJy at 6.75 and 15 micronmetre, respectively. We report the first evidence of an active star-forming region in a cooling flow (at those wavelengths) and strong emission in the mid-IR from lensed galaxies located at z=0.9.
dc.description5 pages, 4 figures. Accepted for publication in Astronomy & Astrophysics Letter. Best resolution figures are available on http://www.mygale.org/~lemonon/article/lw2.ps.gz and http://www.mygale.org/~lemonon/article/lw3.ps.gz
dc.identifierhttps://arxiv.org/abs/astro-ph/9804088
dc.identifierhttp://arxiv.org/abs/astro-ph/9804088
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12321
dc.subjectAstrophysics
dc.titleDeep ISOCAM view of the core of the lensing cluster A2390
dc.typetext

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