RC J0105+0501: A radio galaxy with redshift z≈3.5 View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2000-10

AUTHORS

N. S. Soboleva, W. M. Goss, O. V. Verkhodanov, O. P. Zhelenkova, A. V. Temirova, A. I. Kopylov, Yu. N. Pariiskii

ABSTRACT

We 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... »

PAGES

623-627

Identifiers

URI

http://scigraph.springernature.com/pub.10.1134/1.1316107

DOI

http://dx.doi.org/10.1134/1.1316107

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1027578281


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