Microjansky radio sources in DC0107-46 (Abell 2877)

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dc.creatorHopkins, A.
dc.creatorGeorgakakis, A.
dc.creatorCram, L.
dc.creatorAfonso, J.
dc.creatorMobasher, B.
dc.date2000-01-24
dc.date.accessioned2026-07-07T12:16:19Z
dc.date.available2026-07-07T12:16:19Z
dc.descriptionThe cluster DC0107-46 (Abell 2877) lies within the Phoenix Deep Survey, made at 1.4 GHz with the Australia Telescope Compact Array. Of 89 known optical cluster members, 70 lie within the radio survey area. Of these 70 galaxies, 15 (21%) are detected, with luminosities as faint as 10^20 W/Hz. Spectroscopic observations are available for 14/15 of the radio-detected cluster galaxies. Six galaxies show only absorption features and are typical low-luminosity AGN radio sources. One galaxy hosts a Seyfert 2 nucleus, two are star-forming galaxies, and the remaining five may be star-forming galaxies, AGNs, or both.
dc.description14 pages, 3 figures, Accepted by ApJS (v128n2p JUN 2000 issue)
dc.identifierhttps://arxiv.org/abs/astro-ph/0001413
dc.identifierhttp://arxiv.org/abs/astro-ph/0001413
dc.identifierAstrophys.J.Suppl.128:469-478,2000
dc.identifierdoi:10.1086/313399
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211765
dc.subjectAstrophysics
dc.titleMicrojansky radio sources in DC0107-46 (Abell 2877)
dc.typetext

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