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
Hauptverfasser: Zhang, F. J., Akujor, Chidi E., Chu, H. S., Mutel, R. L., Spencer, R. E., Wilkinson, P. N., Alef, W., Matveyenko, L. I., Preuss, E.
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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.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/250.3.650