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Date and Time of the Query: 2019-06-16 T21:38:02 PDT
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For refcode 2001A&A...380..102M:
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NED Abstract

Copyright by European Southern Observatory (ESO). Reproduced by permission
2001A&A...380..102M A multi-frequency study of the radio galaxy NGC 326 I. The data M. Murgia, P. Parma, H. R. de Ruiter, M. Bondi, R. D. Ekers, R. Fanti and E. B. Fomalont Istituto di Radioastronomia del CNR, via Gobetti 101, 40129, Bologna, Italy Dipartimento di Astronomia, Universita di Bologna, via Ranzani 1, 40127 Bologna, Italy Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia Dipartimento di Fisica, Universita di Bologna, via B. Pichat 6/2, 40127 Bologna, Italy National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 2293, USA Received 10 August 2001/Accepted 5 October 2001 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. Key words: radio continuum: galaxies - galaxies: active - galaxies: individual: NGC 326
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