Very-long-baseline interferometry of compact sources in bright galaxies

Details Very-long-baseline interferometry of compact sources in bright galaxies Very-long-baseline interferometry of compact sources in bright galaxies

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..281c&link_type=abstract

Astronomical Journal, vol. 84, Mar. 1979, p. 281-283.

Astronomy and Astrophysics

Astronomy

29

Galactic Nuclei, Radio Astronomy, Radio Galaxies, Very Long Base Interferometry, Astronomical Spectroscopy, Brightness

Scientific paper

Thirty-one optically bright galaxies with compact radio nuclei have been observed with a 20-million-wavelength baseline at 2380 MHz. Thirteen nuclei have been detected, with angular sizes smaller than 0.01 arcsec. Twelve of the detected nuclei have flat spectra and are about 1 pc, or smaller, in size. This confirms the continuity of properties from the radio nuclei of strong radio galaxies to the less-luminous nuclei of nearby bright galaxies.

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