Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.245..427m&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. Vol. 245, No. 3, p. 427 - 433
Astronomy and Astrophysics
Astronomy
18
Radio Galaxies: Radio Structure, Radio Galaxies: Radio Spectra, Radio Galaxies: Emission Lines
Scientific paper
The authors present VLA, MERLIN and VLBI observations at cm wavelengths of the radio galaxy 3C 99, a low-frequency variable source with a steep radio spectrum. The radio observations show that the source consists of three principal components, which are roughly collinear and have steep radio spectra. Of these, the middle component is the brightest feature at the highest resolutions, has the lowest limits on the degree of polarization and is closest to the position of the optical galaxy. The authors associate this component with the nucleus of the galaxy and suggest that interstellar scattering of the radiation from it could be responsible for the observed low-frequency variability. The two outer components are very asymmetrically located relative to the nucleus, and also differ in peak brightness by a factor of about 70. The authors also present optical spectroscopic observations, made with the Isaac Newton Telescope, which show the presence of extended [O III] emission with a systematic velocity shift of the line across the source. They discuss possible relationships between the extended line emission and the radio structure.
Browne Ian W. A.
Fanti Roberto
Mantovani Fabio
Muxlow Thomas W. B.
Padrielli Lucia
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