A model for far-IR emission of non-Seyfert Markarian galaxies

Details A model for far-IR emission of non-Seyfert Markarian galaxies A model for far-IR emission of non-Seyfert Markarian galaxies

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...225...12x&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 225, no. 1, Nov. 1989, p. 12-26. Research supported by MPI and CNR.

Astronomy and Astrophysics

Astronomy

53

Far Infrared Radiation, H Ii Regions, Infrared Sources (Astronomy), Markarian Galaxies, Astronomical Models, Color-Color Diagram, Grain Size, Infrared Astronomy Satellite, Space Density, Temperature Distribution

Scientific paper

The paper presents simple models for the FIR emission from extended H II regions and from cooler dust heated by the general interstellar radiation field. The models account for a realistic grain-size distribution including PAH molecules. In addition, the model explains the observed correlation between the FIR to optical luminosity ratio and the 60-10 micron colors.

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