Ontology type: schema:ScholarlyArticle
2000-10
AUTHORSN. S. Soboleva, W. M. Goss, O. V. Verkhodanov, O. P. Zhelenkova, A. V. Temirova, A. I. Kopylov, Yu. N. Pariiskii
ABSTRACTWe study the radio galaxy RC J0105+0501 by using observations with RATAN-600, VLA, and 6-m Special Astrophysical Observatory telescope. The radio source has a structure resembling the FRII type and the spectral index α=1.23; it is identified with a faint galaxy of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$22\mathop .\limits^m 8$$ \end{document} in Rc. The optical object is \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} $$1\mathop .\limits^m 5$$ \end{document} brighter in V than it is in B and has an extended structure, which we interpret as intense Lyα line emission with redshift z≈3.5 and a continuum depression in the adjacent short-wavelength region. Based on BVRcIc photometry, we also estimated the age of the stellar population of the radio galaxy. More... »
PAGES623-627
http://scigraph.springernature.com/pub.10.1134/1.1316107
DOIhttp://dx.doi.org/10.1134/1.1316107
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