Combined-array images of an archetypal compact steep-spectrum source, 3C147
We present an EVN map at 1.67 GHz and combined EVN–MERLIN maps at 1.67 and 5 GHz of the compact steep-spectrum radio source 3C147. The maps reveal three dominant extended regions and a bright core. The structure cannot be readily explained with the standard relativistic beaming model. A sharp bend i...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 1991-06, Vol.250 (3), p.650-653 |
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Hauptverfasser: | , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We present an EVN map at 1.67 GHz and combined EVN–MERLIN maps at 1.67 and 5 GHz of the compact steep-spectrum radio source 3C147. The maps reveal three dominant extended regions and a bright core. The structure cannot be readily explained with the standard relativistic beaming model. A sharp bend in the VLBI jet, and the overall distorted structure may be caused by the interaction of the jet with ambient gas, though we cannot rule out a multiengine source each with its own jet. Physical parameters of the knots along the VLBI jet and the age of 3C147 have been estimated. |
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ISSN: | 0035-8711 1365-2966 |
DOI: | 10.1093/mnras/250.3.650 |