RADIO-LUMINOUS SOUTHERN SEYFERT-GALAXIES - I - RADIO IMAGES AND SELECTED OPTICAL NEAR-INFRARED SPECTROSCOPY/

This is the first of two papers in which a study is made of a sample o f 12 southern radio-luminous Seyfert galaxies. Our aim is to investiga te possible correlations between radio morphology and nuclear/circumnu clear emission-line properties. In this paper we present radio images at lambda=13, 6, and 3 cm taken with the Australia Telescope Compact A rray, global far-infrared (FIR) properties for the whole sample, and o ptical and near-infrared spectroscopy of an interesting subset. We fin d a mixture of radio morphologies, including linear, diffuse, and comp act sources. When the FIR colors of the galaxies are considered, there is an indication that the compact radio sources have warmer FIR color s than the diffuse sources, whereas the linear sources span a wide ran ge of FIR colors. There is a wide variation in radio spectral indices, suggesting that free-free absorption is significant in some systems, particularly IRAS 11249 -2859, NGC 4507, and NGC 7213. Detailed emissi on-line studies are presented of four galaxies: IC 3639, NGC 5135, NGC 3393, and IRAS 11249-2859. In IC 3639 we present evidence of vigorous , compact star formation enclosed by very extended [O I] lambda 6300 e mission, suggestive of the boundary between a diffuse outflow and the surrounding interstellar medium. In another galaxy, IC 5063, we see ev idence for the possible interaction of a highly collimated outflow and the surrounding rotating inner disk. Of the five galaxies that show c ompact radio emission, four have radio/FIR flux ratios consistent with an energetically dominant active galactic nucleus, whereas IC 4995 ex hibits evidence for a very compact starburst.