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A multi-frequency study of the radio galaxy NGC 326. I. The data

Astronomy and Astrophysics (2001) 380(1) 102-116
DOI: 10.1051/0004-6361:20011436
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Abstract

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.

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Murgia, M., Parma, P., De Ruiter, H. R., Bondi, M., Ekers, R. D., Fanti, R., & Fomalont, E. B. (2001). A multi-frequency study of the radio galaxy NGC 326. I. The data. Astronomy and Astrophysics, 380(1), 102–116. https://doi.org/10.1051/0004-6361:20011436

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