The radio continuum emission from spiral galaxies in double systems

Details The radio continuum emission from spiral galaxies in double systems The radio continuum emission from spiral galaxies in double systems

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....89l...1h&link_type=abstract

Astronomy and Astrophysics, vol. 89, no. 1-2, Sept. 1980, p. L1, L2. Research supported by the Nederlandse Organisatie voor Zui

Astronomy and Astrophysics

Astrophysics

23

Galactic Radio Waves, Interacting Galaxies, Radio Emission, Spiral Galaxies, Astrophysics, Galactic Nuclei, Galactic Structure, Radio Spectra

Scientific paper

The radio continuum properties of interacting and isolated spiral
galaxies are compared. It is found that the disk emissivity is similar
but that the central sources in interacting galaxies are on the average
a factor 2 to 3 stronger than those in isolated spirals.

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