Microjansky radio sources in DC0107-46 (Abell 2877)

Details Microjansky radio sources in DC0107-46 (Abell 2877) Microjansky radio sources in DC0107-46 (Abell 2877)

2000-01-24

arxiv.org/abs/astro-ph/0001413v1

Astrophys.J.Suppl.128:469-478,2000

Astronomy and Astrophysics

Astrophysics

14 pages, 3 figures, Accepted by ApJS (v128n2p JUN 2000 issue)

Scientific paper

10.1086/313399

The 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.

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