A multi-frequency study of the radio galaxy NGC326
| dc.creator | Murgia, M. | |
| dc.creator | Parma, P. | |
| dc.creator | Fanti, R. | |
| dc.creator | de Ruiter, H. R. | |
| dc.creator | Ekers, R. D. | |
| dc.creator | Fomalont, E. B. | |
| dc.date | 2000-12-06 | |
| dc.date.accessioned | 2026-07-07T01:56:53Z | |
| dc.date.available | 2026-07-07T01:56:53Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012127 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012127 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2169 | |
| dc.subject | Astrophysics | |
| dc.title | A multi-frequency study of the radio galaxy NGC326 | |
| dc.type | text |