The fine structure of 3C 84 and 3C 345 at 18-cm wavelength

Details The fine structure of 3C 84 and 3C 345 at 18-cm wavelength The fine structure of 3C 84 and 3C 345 at 18-cm wavelength

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..148m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Mar. 1982, p. 148-152.) Soviet Astronomy Letters, vol. 8, Mar.-Apr. 1982, p. 77-79.

Astronomy and Astrophysics

Astronomy

3

Fine Structure, Galactic Structure, Radio Galaxies, Radio Sources (Astronomy), Very Long Base Interferometry, Centimeter Waves

Scientific paper

An 18-cm wavelength survey of the angular structure of the radio sources 3C 84 and 3C 345, in which the global radio interferometer network provided approximately 0.0004 arcsec resolution, has revealed a pair of N-S oriented components of 0.0033 arcsec and a pair of compact components, oriented in a 56 deg position angle, which are separated by 0.0026 arcsec. The structure is surrounded by an extended 0.045 arcsec-diameter halo. For 3C 345, the most distinctive features at 18 cm are the presence of a nucleus and two successive jets.

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