A multi-frequency study of the radio galaxy NGC326
Astrophysics
2007-05-23 v1
Abstract
We present preliminary results of a multi-frequency study of the inversion symmetric radio galaxy NGC326 based on VLA observations at 1.4, 1.6, 4.8, 8.5, and 14.9 GHz. These data allow us to investigate in detail the morphological, spectral and polarization properties of this peculiar object at different levels of spatial resolution.
Cite
@article{arxiv.astro-ph/0012127,
title = {A multi-frequency study of the radio galaxy NGC326},
author = {M. Murgia and P. Parma and R. Fanti and H. R. de Ruiter and R. D. Ekers and E. B. Fomalont},
journal= {arXiv preprint arXiv:astro-ph/0012127},
year = {2007}
}
Comments
4 pages, 3 figures, uses newpasp.sty (included). To appear in R.A. Laing and K.M. Blundell (Eds.) 'Particles and Fields in Radio Galaxies' Oxford, UK, 2000, to be published by the Astronomical Society of the Pacific (ASP)