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AbstractAbstract
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Astronomical Journal; v. 77(1); p. 13-16
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AbstractAbstract
[en] The components of powerful extragalactic radio sources show a characteristic head-tail structure. If synchrotron losses play a major part in limiting the lengths of the tails, the tails should be longer at low frequencies than at high frequencies. New observations of 3C172 indicate that such differences are not observed, and this conclusion is consistent with published data on other sources. (author)
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Journal Article
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Monthly Notices of the Royal Astronomical Society; v. 174(2); p. 327-333
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Shaffer, D.B.
California Inst. of Tech., Pasadena (USA)1974
California Inst. of Tech., Pasadena (USA)1974
AbstractAbstract
No abstract available
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1974; 106 p; University Microfilms Order No. 74-14,285.; Thesis (Ph. D.).
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Report
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Thesis/Dissertation
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AbstractAbstract
[en] Accurate radio positions and optical identifications are presented for some sources from the Ohio survey. (1 figure, 1 table, 10 references) (U.S.)
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Journal Article
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Publications of the Astronomical Society of the Pacific; v. 87(515); p. 103-106
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AbstractAbstract
[en] Examination of the structures of extragalactic radio sources shows a distinct asymmetry in addition to the more general symmetries which are well known. The most likely explanation for the observed asymmetries is that ejection from the active nucleus occurs in only one direction at a time. This direction then switches back and forth to form the large scale double structures. Implications of this picture for the nuclear engine and the radio source environment are discussed. (Auth.)
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Heeschen, D.S.; Wade, C.M. (National Radio Astronomy Observatory, Charlottesville, VA (USA)) (eds.); International Astronomical Union symposium; no. 97; 506 p; ISBN 90-277-1384-7;
; 1982; p. 47-49; D. Reidel; Dordrecht, Netherlands; 97. International Astronomical Union symposium on extragalactic radio sources; Albuquerque, USA; 3 - 7 Aug 1981

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AbstractAbstract
No abstract available
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Journal Article
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Astrophysical Journal; v. 174(3); p. L111-L114
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AbstractAbstract
[en] Photoelectric observations of eight optically identified radio sources and comparison stars in nearby fields are presented. Six of these objects have continuous spectra and may belong to the BL Lac class of variables. The reported observations indicate possible short-term, small-amplitude variations in some of the optical counterparts of the radio sources. (9 figures, 3 tables, 14 references) (U.S.)
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Journal Article
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Publications of the Astronomical Society of the Pacific; v. 87(515); p. 123-130
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AbstractAbstract
No abstract available
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Letter to the editor.
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Journal Article
Journal
Nature (London); v. 255(5506); p. 310-312
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AbstractAbstract
[en] A formula for the surface brightness of an optically thin radio jet is presented and compared to observations for NGC 315. (Auth.)
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Source
Heeschen, D.S.; Wade, C.M. (National Radio Astronomy Observatory, Charlottesville, VA (USA)) (eds.); International Astronomical Union symposium; no. 97; 506 p; ISBN 90-277-1384-7;
; 1982; p. 227-228; D. Reidel; Dordrecht, Netherlands; 97. International Astronomical Union symposium on extragalactic radio sources; Albuquerque, USA; 3 - 7 Aug 1981

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Book
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Komesaroff, M.M.; Milne, D.K.; Rayner, P.T.; Roberts, J.A.; Cooke, D.J.
Extragalactic radio sources1982
Extragalactic radio sources1982
AbstractAbstract
[en] Observations for four sample sources from the Parkes 5 GHz polarization monitoring programme are presented and the interesting features are discussed. These include sudden changes of the position angle of the polarization, linear increase in the position angle of polarization and distinct burst of circular polarization. (Auth./C.F.)
Primary Subject
Source
Heeschen, D.S.; Wade, C.M. (National Radio Astronomy Observatory, Charlottesville, VA (USA)) (eds.); International Astronomical Union symposium; no. 97; 506 p; ISBN 90-277-1384-7;
; 1982; p. 331-333; D. Reidel; Dordrecht, Netherlands; 97. International Astronomical Union symposium on extragalactic radio sources; Albuquerque, USA; 3 - 7 Aug 1981

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Book
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