Other
Scientific paper
Jan 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219...77g&link_type=abstract
Astrophysical Journal, Part 1, vol. 219, Jan. 1, 1978, p. 77-94.
Other
86
Emission Spectra, Interstellar Gas, Sulfur Oxides, Abundance, Cosmic Dust, Electron Transitions, H Ii Regions, Interstellar Matter, Sulfur Dioxides
Scientific paper
In the reported investigation involving a number of sources, SO emission features were compared with those of other sulfur-containing species including CS, NS, SiS, OCS, SO2, H2S, and H2CS. The sources considered included molecular clouds associated with H II regions, dust clouds, and Ae and Be stars. Six transitions were observed of SO containing S-32 and two transitions of SO containing S-34. It is pointed out that the transitions of SO containing S-34 observed toward the Kleinmann-Low nebula are about as strong as predicted from the terrestrial S-34/S-32 abundance ratio. The velocity, width, and general source distribution of SO, H2S, and CS emission features are closely correlated (except toward the Kleinmann-Low nebula, where no CS is reported). The predictions of the ion-molecule theory agree well with the observed abundances of NS, OCS, and H2S relative to SO.
Ball Joseph A.
Gottlieb Carl A.
Gottlieb E. W.
Litvak Marvin M.
Penfield Hays
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