Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..566c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 283, Aug. 15, 1984, p. 566-572. Research supported by Colby College.
Astronomy and Astrophysics
Astronomy
1
Emission Spectra, Infrared Astronomy, Interstellar Matter, Milky Way Galaxy, Radio Sources (Astronomy), Astronomical Maps, Brightness Temperature, Far Infrared Radiation, H Ii Regions, Luminosity, Molecular Clouds, Submillimeter Waves
Scientific paper
Medium resolution (11 min) maps of the galactic plane are presented from l = 11.5 deg to l = 17.5 deg at wavelengths of 93 microns, 154 microns, and 190 microns. The maps are interpreted in terms of the temperature and spatial structure of diffuse far-infrared/submillimeter sources associated with evolved H II regions and a continuous ridge of galactic emission. The emission regions are found to be more extended at the longer wavelengths which implies that there must be a range of dust temperatures in the sources. The properties of the galactic ridge are similar to those of the sources.
Campbell Marvin F.
Hauser Michael G.
Hoffmann William F.
Kelsall Thomas
Niles David W.
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