期刊
ASTRONOMICAL JOURNAL
卷 123, 期 6, 页码 2985-2989出版社
UNIV CHICAGO PRESS
DOI: 10.1086/340359
关键词
galaxies : active; galaxies : clusters : individual (4U 0446+44); galaxies : jets
We present a new wide-field map of the radio galaxy 3C 129 and its companion galaxy 3C 129.1 at lambda = 90 cm. We see a distinct steep-spectrum feature near the head of 3C 129, extending in a direction perpendicular to the radio tails. We propose that this Crosspiece might consist of fossil radio plasma, which has been re-energized by the compression of the bow shock of the supersonically moving galaxy 3C 129. One possible origin of the fossil radio plasma could be the tail of a nearby head-tail radio galaxy. We discuss the implications of and give testable predictions for this scenario.
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