40-350 micron observations of galactic sources

40-350 micron observations of galactic sources

Broad-band 40--350 $mu$ measurements are reported for 31 sources observed with a balloon-borne telescope. All but one of the sources have been identified with galactic H ii regions, of which about one-third are optically visible. The objects include W3 (three components), W49, RCW 36, RCW 38, and 24...

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Veröffentlicht in:Astrophys. J., v. 202, no. 2, pp. 400-406 v. 202, no. 2, pp. 400-406, 1975-12, Vol.202, p.400
Hauptverfasser: Furniss, I., Jennings, R. E., Moorwood, A. F. M.
Format: Artikel
Sprache:eng
Schlagworte:
640105 -Physics Research-Astrophysics & Cosmology- Galaxies
COSMIC DUST
H2 REGIONS
INTERSTELLAR GRAINS
N56500 -Physics (Astrophysics & Cosmology)-Galaxies
NEBULAE- FAR INFRARED RADIATION
PHOTOMETRY
RESOLUTION
SPECTRA
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Zusammenfassung:Broad-band 40--350 $mu$ measurements are reported for 31 sources observed with a balloon-borne telescope. All but one of the sources have been identified with galactic H ii regions, of which about one-third are optically visible. The objects include W3 (three components), W49, RCW 36, RCW 38, and 24 sources lying along the galactic plane between l/sup II/=327degree and 349degree. Most of these sources have not previously been observed in the far-infrared. A contour map of the W3 region shows an emission arm extending from the main continuum component. (AIP)
ISSN:0004-637X
1538-4357
DOI:10.1086/153988