Contribution of the warm intercloud medium to the diffuse ultraviolet background

Details Contribution of the warm intercloud medium to the diffuse ultraviolet background Contribution of the warm intercloud medium to the diffuse ultraviolet background

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...109..179d&link_type=abstract

Astronomy and Astrophysics, vol. 109, no. 1, May 1982, p. 179-181.

Astronomy and Astrophysics

Astrophysics

13

Background Radiation, Diffuse Radiation, Galactic Radiation, Ultraviolet Radiation, B Stars, Brightness, H Ii Regions, Hydrogen Ions, Line Spectra, O Stars

Scientific paper

The far UV emission from the warm intercloud medium (mainly two photon
continuum and emission lines) is evaluated and compared to observations
of the diffuse UV radiation. Whereas this emission may account for the
UV surface brightness of faint extended H II regions, it is found unable
to contribute significantly to the general diffuse UV background.

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