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2002MNRAS.331..673S - Mon. Not. R. Astron. Soc., 331, 673-683 (2002/April-2)
Shocks, illumination cones and intrinsic gas structures in the extreme radio galaxy 3C265.
SOLORZANO-INARREA C., TADHUNTER C.N. and BLAND-HAWTHORN J.
Abstract (from CDS):
Our images show that, while on a large scale the low-ionization emission-line structures are aligned with the radio axis, on a smaller scale, where AGN-photoionization dominates, the highest surface-brightness structure is aligned with the closest companion galaxy (misaligned with the radio axis). This suggest that much of the emission-line structure reflects the intrinsic gas distribution, rather than the ionization pattern imprinted by the radio jets or by illumination from the central AGN.
Overall, our results underline the need for a variety of mechanisms to explain the properties of the extended emission-line gas in the haloes of radio galaxies.
Abstract Copyright: 2002 Blackwell Science Ltd
Journal keyword(s): galaxies: active - galaxies: individual: 3C265 - galaxies: jets - galaxies: kinematics and dynamics - galaxies: structure
CDS comments: p.675: Standard star SP 1337+705 = WD 1337+705
Simbad objects: 13
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