Enhanced star formation in barred spiral galaxies. II - Radio continuum emission

Astronomy and Astrophysics – Astronomy

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Astronomical Spectroscopy, Barred Galaxies, Radio Emission, Star Formation, Continuous Spectra, Data Sampling, Far Infrared Radiation, Infrared Astronomy Satellite, Morphology

Scientific paper

The radio properties of an IRAS-selected sample of nearby spiral galaxies have been investigated using new and published 20-cm continuum observations. Virtually all of the galaxies with steep 12 - 25 μm spectra are barred and possess a central radio source of linear extent less than 1 - 3 kpc. The authors argue that the activity in these systems is due to enhanced star formation rather than a compact nucleus. The central sources contribute, on average, 35 per cent to the total radio emission and their typical far-infrared luminosity is estimated to be a few ×109L_sun;. In contrast to the other IRAS wavebands, the 25 μm-radio correlation shows a marked dependence on the level of star-formation activity.

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