Evolutionary synthesis of the far-infrared emission in starburst galaxies

Details Evolutionary synthesis of the far-infrared emission in starburst galaxies Evolutionary synthesis of the far-infrared emission in starburst galaxies

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..501m&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 501-506 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

Far Infrared Radiation, Galactic Evolution, Infrared Spectra, Starburst Galaxies, Astronomical Models, Cosmology, Emission Spectra, Star Distribution, Star Formation

Scientific paper

The evolutionary population synthesis models are used to study the Far Infrared (FIR) emission in star forming galaxies. The dust particles, heated by the energetic photons (originated in the young massive stars), reradiate the energy thermally in the FIR. The models can explain the tight correlation between the FIR and the radio emission actually observed. Both the thermal and the non-thermal contribution to the radio continuum are considered. The time evolution of the ratio FIR/LH beta is studied. It appears to be a good age indicator.

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