The structure of the quasar 3C 345 at a wavelength of 49 CM

Details The structure of the quasar 3C 345 at a wavelength of 49 CM The structure of the quasar 3C 345 at a wavelength of 49 CM

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..579m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, July 1990, p. 579-597. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Quasars, Radio Sources (Astronomy), Stellar Structure, Very Long Base Interferometry, Brightness Temperature, Fine Structure, Radio Astronomy, Stellar Cores

Scientific paper

A study of the structure of the quasar 3C 345 was conducted at 49 cm using the global VLBI network. Compact components are distributed mainly along the jet; a counterjet region is also observed. The maximum brightness temperature of the compact regions is Tb less than 10 to the 12th K, and it is suggested that the curvature of the jet is probably due to the rotation of the nucleus, whose angular velocity is increasing.

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