Polarimetry of the ultraviolet continua of southern radio galaxies
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-08-01 and is currently open access. It has received 16 citations till now. The article focuses on the topics: X-shaped radio galaxy & Radio galaxy.read more
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Journal ArticleDOI
The Compact Steep-Spectrum and Gigahertz Peaked-Spectrum Radio Sources
TL;DR: In this article, the radio to X-ray properties of GPS and CSS sources are reviewed and the current hypotheses for their origin and their use to constrain the evolution of powerful radio galaxies.
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Radio AGN in the local universe: unification, triggering and evolution
TL;DR: In this paper, the authors review the current state of understanding of the population of radio active galactic nucleus (AGN) at low and intermediate redshifts, focusing on their nuclear AGN and host galaxy properties.
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Starbursts and the triggering of the activity in nearby powerful radio galaxies
TL;DR: In this article, the authors present high-quality long-slit spectra for three nearby powerful radio galaxies (3C 293, 3C 305 and PKS 1345+12) with the aim of characterizing the young stellar populations (YSP), and thereby investigating the evolution of the host galaxies, as well as the events that triggered the activity.
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The origin of the UV excess in powerful radio galaxies: spectroscopy and polarimetry of a complete sample of intermediate‐redshift radio galaxies
Clive Tadhunter,R. Dickson,Raffaella Morganti,T. G. Robinson,K. A. Wills,M. Villar-Martin,M. Hughes +6 more
TL;DR: In this article, the authors present spectroscopic and polarimetric observations of a complete, optically unbiased sample of 2-Jy radio galaxies at intermediate redshifts (0.15 10 per cent level).
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H i absorption in radio galaxies: effect of orientation or interstellar medium?
TL;DR: In this article, the authors investigated how the detection rate is distributed among radio galaxies with different radio and optical properties, and they found that the most likely cause of H-I absorption in radio galaxies is likely to come from a nuclear disc.