NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-08-18 T00:46:13 PDT
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For refcode 2000ApJS..128..469H:
Retrieve 16 NED objects in this reference.
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NED Abstract

Copyright by American Astronomical Society. Reproduced by permission
2000ApJS..128..469H Microjansky Radio Sources in DC 0107-46 (Abell 2877) A. Hopkins Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 A. Georgakakis School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK L. Cram School of Physics, University of Sydney, NSW 2006, Australia and J. Afonso and B. Mobasher Astrophysics Group, The Blackett Laboratory, Prince Consort Road, London SW7 2BZ, UK Received 1999 December 24; accepted 2000 January 24 ABSTRACT The cluster DC 0107-46 (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 1.0 x 10^20^ W Hz^-1^. Spectroscopic observations are available for 14/15 of the radio- detected cluster galaxies. Six galaxies show only absorption features and are typical low-luminosity active galactic nucleus (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. Subject headings: galaxies: clusters: individual (Abell 2877)-galaxies: evolution-galaxies: starburst-radio continuum: galaxies
Retrieve 16 NED objects in this reference.
Please click here for ADS abstract

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