The identification of galactic radio sources based on a comparison of radio-continuum and infrared emission

Details The identification of galactic radio sources based on a comparison of radio-continuum and infrared emission The identification of galactic radio sources based on a comparison of radio-continuum and infrared emission

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...71...63f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 71, no. 1, Oct. 1987, p. 63-67.

Astronomy and Astrophysics

Astronomy

49

Continuous Spectra, Galactic Radiation, Infrared Spectra, Radio Sources (Astronomy), Radio Spectra, Spectrum Analysis, Emission Spectra, Hydrogen Clouds, Nonthermal Radiation, Supernova Remnants, Thermal Radiation

Scientific paper

The ratio of the far-infrared to the radio continuum emission is very different for H II regions and supernova remnants. Using the IRAS 60 μm and radio 2.7 GHz emission it is demonstrated that this difference provides an effective tool to distinguish between thermal and non-thermal sources even in highly confused regions in the galactic plane.

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