Jets, plumes and hotspots in the wide-angle tail source 3C 130 |
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Authors: | M. J. Hardcastle |
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Affiliation: | H. H. Wills Physics Laboratory, University of Bristol, Royal Fort, Tyndall Avenue, Bristol BS8 1TL,;Mullard Radio Astronomy Observatory, Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE |
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Abstract: | I present 1.5- and 8.4-GHz observations with all configurations of the NRAO VLA of the wide-angle tail source 3C 130. The source has a pair of relatively symmetrical, well-collimated inner jets, one of which terminates in a compact hotspot. Archival ROSAT PSPC data confirm that the environment of 3C 130 is a luminous cluster with little sign of sub-structure in the X-ray-emitting plasma. I compare the source to other wide-angle tail objects and discuss the properties of the class as a whole. None of the currently popular models is entirely satisfactory in accounting for the disruption of the jets in 3C 130. |
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Keywords: | galaxies: active galaxies: individual: 3C 130 galaxies: jets radio continuum: galaxies |
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