Radio-far-infrared relation in Markarian galaxies

Details Radio-far-infrared relation in Markarian galaxies Radio-far-infrared relation in Markarian galaxies

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...281..718m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 281, no. 3, p. 718-724

Astronomy and Astrophysics

Astronomy

13

Comparison, Far Infrared Radiation, Infrared Astronomy, Markarian Galaxies, Radio Astronomy, Radio Emission, Starburst Galaxies, Astronomical Spectroscopy, Correlation, Flux Density, Quasars, Seyfert Galaxies, Stellar Luminosity

Scientific paper

We have compared the radio continuum properties of Markarian galaxies at lambda lambda 6.3 and 2.8 cm with the integrated far-infrared luminosities over the 60 micrometer and 100 micrometer IRAS bands and over the 12 micrometer to 25 micrometer regime. We find that Markarian galaxies behave like normal star-forming galaxies. Comparing L60, 100 with the radio emission, most objects lie in the region of normal star-forming galaxies. Only some Seyferts and most of the radio-quiet quasars show a higher radio-to-FIR ratio. Comparing L12, 25 with the radio luminosity, the correlation is surprisingly tight for all objects. In both cases the dispersion of the correlation seems to depend on the radio wavelength and is smaller at lambda 2.8 cm than at lambda 6.3 cm.

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