Does the far-infrared/radio correlation in spiral galaxies extend to the spatial domain?

Details Does the far-infrared/radio correlation in spiral galaxies extend to the spatial domain? Does the far-infrared/radio correlation in spiral galaxies extend to the spatial domain?

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.345h&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 345 - 346

Physics

Spiral Galaxies: Infrared Radiation, Spiral Galaxies: Radio Radiation

Scientific paper

A comparison is made between the spatial distribution of the thermal far-infrared and non-thermal radio emission of nearby spiral galaxies. A physical explanation for this correlation is not straight forward due to the ambiguous nature of the origin of the far-infrared and radio, and the dependence of the non-thermal radio on each galaxies' magnetic field.

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