Abstract
Based on data from the MIT-GB-VLA 4850-MHz survey, we investigate the radio structure of RC J1148+0455 with a steep radio spectrum (α=−1.04) from the COLD catalog. The radio source consists of two components, each having a complex structure. We analyze an optical identification of the source by using 6-m telescope images. The centroid of the radio source falls on a group of eight galaxies at a 24m level in R.
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Translated from Pis’ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 26, No. 7, 2000, pp. 493–498.
Original Russian Text Copyright © 2000 by Pari\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \)ski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \), Soboleva, Kopylov, Verkhodanov, Temirova, Zhelenkova, Winn, Fletcher, Burke.
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Pariiskii, Y.N., Soboleva, N.S., Kopylov, A.I. et al. The radio galaxy RC J1148+0455. Astron. Lett. 26, 423–427 (2000). https://doi.org/10.1134/1.20410
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DOI: https://doi.org/10.1134/1.20410