Volume 380, Number 1, December II 2001
|Page(s)||102 - 116|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 December 2001|
A multi-frequency study of the radio galaxy NGC 326
I. The data
Istituto di Radioastronomia del CNR, via Gobetti 101, 40129, Bologna, Italy
2 Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
3 Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
4 Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia
5 Dipartimento di Fisica, Università di Bologna, via B. Pichat 6/2, 40127 Bologna, Italy
6 National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 2293, USA
Corresponding author: M. Murgia, email@example.com
Accepted: 5 October 2001
We present the results of a multi-frequency study of the inversion symmetric radio galaxy NGC 326 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.
Key words: radio continuum: galaxies / galaxies: active / galaxies: individual: NGC 326
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.