Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....96...58g&link_type=abstract
Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 58-63.
Astronomy and Astrophysics
Astronomy
12
Galactic Radio Waves, Radiant Flux Density, Radio Astronomy, Radio Emission, Spiral Galaxies, Galactic Structure, Hubble Diagram, Optical Properties, Radio Galaxies
Scientific paper
The bivariate radio luminosity function for spiral galaxies has been derived. It shows that higher radio powers are found for galaxies of higher optical luminosity. The dependence of the radio emission on various optical parameters (i.e. Hubble classification, luminosity class, etc.) is examined. From the comparison of the radio emission properties of group and field galaxies, there is an indication that galaxies in groups have a lower probability of being radio sources than field galaxies.
Gioia Isabella Maria
Gregorini Loretta
Vettolani Giampaolo
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