Multifrequency Study of The Radio Galaxy NGC326
Astrophysics
2009-11-07 v1
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.
Cite
@article{arxiv.astro-ph/0110252,
title = {Multifrequency Study of The Radio Galaxy NGC326},
author = {M. Murgia and P. Parma and H. R. de Ruiter and M. Bondi and R. D. Ekers and R. Fanti and E. B. Fomalont},
journal= {arXiv preprint arXiv:astro-ph/0110252},
year = {2009}
}
Comments
15 pages, 15 ps figures, accepted by A&A