Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392l..35r&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 392, no. 1, June 10, 1992, p. L35-L38.
Astronomy and Astrophysics
Astrophysics
79
Background Radiation, Emission Spectra, Interstellar Matter, Line Spectra, Milky Way Galaxy, Infrared Radiation, Millimeter Waves, Radio Spectra, Ultraviolet Radiation
Scientific paper
High-latitude H-alpha line data and the resulting predicted intensities of the associated FUV and millimeter continuum emissions and the IR lines are presented. The emissions predicted account for all of the diffuse forbidden N II FIR line emission at high latitudes, about 20 percent of the observed FUV continuum, and about 1- exp -6 to 10 exp -5 of the microwave background near the peak of the 2.73 K blackbody spectrum, where the free-free intensity is comparable to that of the synchrotron and thermal dust emission. The angular structure in the Ha-alpha background implies the existence of high-altitude features with intensities about a factor of 2 above these average values.
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