Enhanced radio emission in binary spiral galaxies

Details Enhanced radio emission in binary spiral galaxies Enhanced radio emission in binary spiral galaxies

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1531a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, Oct. 1984, p. 1531-1535.

Astronomy and Astrophysics

Astronomy

20

Galactic Radio Waves, Gravitational Effects, Radio Galaxies, Spiral Galaxies, Astronomical Catalogs, Luminous Intensity, Radio Emission, Tides

Scientific paper

A comparison is conducted between the radio emission characteristics of a sample of isolated pairs of spiral galaxies and those of a sample of isolated spiral galaxies for which complete distance information is available. It is noted that double galaxy total emission is, on average, a factor of 2 more powerful than that of isolated spiral galaxies of comparable luminosity. The radio emission enhancement in these double galaxies is correlated with a tidal index, in keeping with a tidal origin for the enhancement.

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