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Studies of the 3c 345 Quasar Structure at Dm-Wavelengths

Matveyenko, L.I. (author)
Space Research Institute, Russian Academy of Sciences, Moscow, Russia
Pauliny-Toth, I.I.K. (author)
Max-Planck-Institute für Radio Astronomie, Bonn, Germany
Sherwood, B. (author)
Max-Planck-Institute für Radio Astronomie, Bonn, Germany
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Bååth, L.B. 1948- (author)
Onsala Space Observatory, Chalmers University of Technology, Gothenburg, Sweden
Kus, A. (author)
Torun Radio Astronomy Observatory, Torun, Poland
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 (creator_code:org_t)
Dordrecht : D. Reidel Publishing Group, 1987
1987
English.
In: Observational evidence of activity in galaxies. - Dordrecht : D. Reidel Publishing Group. - 9027724733 - 9027724741 ; , s. 301-304
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • The structure of the quasar 3C 345 has been studied at 18 and 49 cm wavelengths by VLBI method. The structure has a nucleus and a jet, which changes direction with distance from the nucleus. The continuum emission of the nucleus and the jet regions correspond to a source with a large optical depth, the cut frequence goes down with increasing distance from nucleus.

Subject headings

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

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