Abstract
3C 390 ·3 has been mapped at 2 ·7 and 5 GHz with the Cambridge One-Mile telescope. It is found to consist of three compact components and an extended region of emission. The central component, not previously detected, is coincident with the associated N -galaxy and has a spectral cut-off below about 3 GHz. Maps of the polarized emission have also been obtained and provide information on physical conditions in the source.

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