Evolutionary synthesis of the radio and far-infrared emission in starbursts

Details Evolutionary synthesis of the radio and far-infrared emission in starbursts Evolutionary synthesis of the radio and far-infrared emission in starbursts

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253...49m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 1, Jan. 1992, p. 49-56. Research supported by ESA and DGICYT.

Astronomy and Astrophysics

Astrophysics

15

Far Infrared Radiation, Galactic Evolution, Galactic Radiation, Radio Galaxies, Starburst Galaxies, Supernova Remnants, Compact Galaxies, Dwarf Galaxies, H Ii Regions, Interacting Galaxies, Luminous Intensity, Spiral Galaxies, Star Formation

Scientific paper

A reanalysis of the correlation between the radio and far-IR luminosities in a sample of 230 objects with active star formation from the literature indicates that simple evolutionary-synthesis models can generally reproduce the observed ratio R between radio and far-IR emission, as well as the radio spectral index. The thermal radio excess found in LMC H II regions and blue compact dwarf galaxies suggests that the ionizing flux emitted by a metal-deficient cluster of young massive stars is significantly higher than at solar metallicities.

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