On the observed infrared fluxes from extragalactic H II regions

Details On the observed infrared fluxes from extragalactic H II regions On the observed infrared fluxes from extragalactic H II regions

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..50...87i&link_type=abstract

Astrophysics and Space Science, vol. 50, no. 1, Aug. 1977, p. 87-92.

Astronomy and Astrophysics

Astrophysics

Extragalactic Radio Sources, Granular Materials, H Ii Regions, Infrared Radiation, Thermal Emission, Astronomical Models, Graphite, Hydrogen Ions, Radiant Flux Density

Scientific paper

The paper describes the calculations for extragalactic H II regions of the expected relationship between the radio flux at 11 cm and the IR flux at 11 and 20 microns. These calculations are based on grain models and the parameters which fit the observations of galactic H II regions. Graphite and silicon grain models were compared, and the results are more in accord with the graphite model. It is shown that the measured IR fluxes of extragalactic H II regions are consistent with the expected IR fluxes for these objects.

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