Radio Continuum Emission from Magellanic-Type and Dwarf Irregular Galaxies

Details Radio Continuum Emission from Magellanic-Type and Dwarf Irregular Galaxies Radio Continuum Emission from Magellanic-Type and Dwarf Irregular Galaxies

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..313k&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

1

Scientific paper

High-frequency radio continuum observations of a small sample of
irregular and dwarf galaxies have revealed that their integrated radio
continuum spectra tend to be significantly flatter than those found for
normal spirals. This indicates a higher relative amount of thermal
(free-free) emission.

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