Radio continuum emission in nearby non-cluster spirals

Details Radio continuum emission in nearby non-cluster spirals Radio continuum emission in nearby non-cluster spirals

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...195....9g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 195, no. 1-2, April 1988, p. 9-14. Research supported by the Ministero della P

Astronomy and Astrophysics

Astrophysics

4

Continuous Radiation, Radio Emission, Radio Galaxies, Spiral Galaxies, Virgo Galactic Cluster, H Alpha Line, H I Regions, Star Formation Rate

Scientific paper

Examining the radio continuum properties of ≡200 nearby non-cluster spirals, the authors have found that the radio continuum emission (per unit light) of spirals is (a little) linked to their colour indices (U-B)0T and (more closely) to their Hα emission strengths, but not to indices of H I content. There appears to be no dependence of the radio power of the spiral members of galaxy groups on the group compactness. However, within a sample of interacting spirals, enhanced radio emission is observed in the most strongly interacting systems.

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