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VLBI Observations of 3C345 at 1.67 GHz

Stannard, D. (author)
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Cheshire, UK
Booth, R.S. (author)
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Cheshire, UK
Spencer, R.E. (author)
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Cheshire, UK
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Bååth, L.B. 1948- (author)
Onsala Space Observatory, Chalmers Institute of Technology, Gothenburg, Sweden
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 (creator_code:org_t)
Oxford : Oxford University Press, 1980
1980
English.
In: Monthly notices of the Royal Astronomical Society. - Oxford : Oxford University Press. - 0035-8711 .- 1365-2966. ; 192:4, s. 555-560
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  • VLBI observations of the quasar 3C 345 suggest that the milliarcsec subcomponents in the core have approximately equal intensities at 1.67 GHz. A new compact feature is detected in the inner jet structure at a distance of ∼ 12 m.arcsec from the core. © 1980 Royal Astronomical Society. Provided by the NASA Astrophysics Data System

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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Spencer, R.E.
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Halmstad University

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