Multifrequency Study of The Radio Galaxy NGC326

Abstract

We present the results of a multi-frequency study of the inversion symmetric radio galaxy NGC326 based on Very Large Array observations at 1.4, 1.6, 4.8, 8.5 and 14.9 GHz. The morphological, spectral and polarization properties of this peculiar object are studied at different levels of spatial resolutions. The interpretation of the data will be discussed in forthcoming papers.

15 pages, 15 ps figures, accepted by A&A

References in corpus (2)

• X-ray-emitting Atmospheres of B2 Radio Galaxies
• Redshift and velocity dispersion of the cluster of galaxies around NGC 326

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