The Core of Cluster-Lenses

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dc.creatorKneib, J. -P.
dc.creatorSoucail, G.
dc.date1995-10-08
dc.date.accessioned2026-07-07T02:20:16Z
dc.date.available2026-07-07T02:20:16Z
dc.descriptionThe gravitational lensing of faint background galaxies by rich clusters is emerging as a very efficient method to constrain both the mass distribution of cluster of galaxies and probe the statistical properties of faint background galaxies. We review here the results concerning the core of cluster lenses, where recent Hubble Space Telescope (HST) images are giving a new insight in the gravitational distortion phenomena.
dc.descriptionuuencoded compressed postscript. The preprint is also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9510048
dc.identifierhttp://arxiv.org/abs/astro-ph/9510048
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10162
dc.subjectAstrophysics
dc.titleThe Core of Cluster-Lenses
dc.typetext

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