A radio continuum survey of nearby galaxies. I - Observations at 0.4, 0.8, 4.8, and 10.7 GHz

Astronomy and Astrophysics – Astronomy

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Continuous Spectra, Galactic Radio Waves, Radio Galaxies, Radio Spectra, Spiral Galaxies, Thermal Emission, Astronomical Maps, Centimeter Waves, Elliptical Galaxies, Radiant Flux Density

Scientific paper

The authors have observed a total of 136 galaxies at one or more of four frequencies: 430, 834, 4750, and 10700 MHz. For a subset of these, spectral indices could be determined. The authors find a mean value α = -0.68±0.04 (Sν ∝ να) over the whole frequency range covered. The mean high frequency spectral index (4.9 - 10.7 GHz) for Sc galaxies is α = -0.55±0.07, which indicates the presence of significant amounts of thermal emission in a considerable fraction of the sample. At 10.7 GHz the mean thermal contribution to the radio emission of the sample Sc galaxies is 35±15 per cent; for the sample Sb galaxies this is 20±15 per cent.

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