The radio brightness distribution of eight Markarian galaxies

Details The radio brightness distribution of eight Markarian galaxies The radio brightness distribution of eight Markarian galaxies

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207..725s&link_type=abstract

Astrophysical Journal, vol. 207, Aug. 1, 1976, pt. 1, p. 725-729, 731, 733, 735.

Astronomy and Astrophysics

Astronomy

35

Galactic Radiation, Luminous Intensity, Markarian Galaxies, Radio Sources (Astronomy), Seyfert Galaxies, Galactic Nuclei, Spectral Energy Distribution, Ultraviolet Radiation

Scientific paper

Results of radio aperture-synthesis observations at 2.7 and 8.1 GHz are given for eight Markarian galaxies. Five of these galaxies are Seyfert-type objects (MRK 1, 3, 231, 273, and 348) and one is a BL Lacertae object (MRK 501); these exhibit only an unresolved radio nucleus. Two other galaxies show an extended source (MRK 297) and a double source inside the optical image (MRK 171). This double source coincides with optically bright regions that are off-center with respect to the general outline of the galaxy.

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