Faint Field Galaxies: A Population of Intrinsically Faint Objects at Low Redshift?

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dc.creatorCampos, Ana
dc.date1994-11-30
dc.date.accessioned2026-07-07T02:19:37Z
dc.date.available2026-07-07T02:19:37Z
dc.descriptionTo distinguish between the different models proposed to understand the excess of faint field counts over the predictions from non-evolving models, a number of redshift surveys have been undertaken. The answer has not arrived yet due to the high rate of incompleteness achieved. Un-identified galaxies have been shown to be bluer than identified ones. In this paper, it is argued that some of these galaxies could be "quiescent" dwarfs, still quite blue, but with featureless spectra.
dc.description5 pages 2 Figures, uuencoded compressed Postscript. To appear in the Proceedings of the 11th Internation Potsdam Workshop on Large Scale Structure in The Universe
dc.identifierhttps://arxiv.org/abs/astro-ph/9411115
dc.identifierhttp://arxiv.org/abs/astro-ph/9411115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9934
dc.subjectAstrophysics
dc.titleFaint Field Galaxies: A Population of Intrinsically Faint Objects at Low Redshift?
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