Radio continuum observations of Markarian Galaxies at 1410, 2380, and 5000 MHz

Details Radio continuum observations of Markarian Galaxies at 1410, 2380, and 5000 MHz Radio continuum observations of Markarian Galaxies at 1410, 2380, and 5000 MHz

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81..235b&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 1-2, Jan. 1980, p. 235-239. Research supported by the National Research Council of Can

Astronomy and Astrophysics

Astronomy

44

Bl Lacertae Objects, Galaxies, Markarian Galaxies, Radio Astronomy, Seyfert Galaxies, Astronomical Catalogs, Spectrum Analysis, Telescopes, Ultraviolet Spectra

Scientific paper

Markarian Galaxies were observed with the 100 m Effelsberg and the 305 m Arecibo telescopes. The ratio of radio power and blue light plotted against B-V shows that all galaxies which are neither variable nor BL Lac objects, lie close to or below the limiting reddening line for bursts of star formation with the exception of MRK011 which has a flat spectrum and is suspected to be a BL Lac object. The earlier conclusion (Biermann and Fricke, 1977; Bieging et al., 1977) that bursts of star formation can explain the radio radiation and the colors of many Markarian galaxies is confirmed.

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