
doi: 10.1086/185553 , 10.7275/2397
pmid: 11538326
Interstellar H2S has been detected toward the cold, dark clouds L134N and TMC 1. Total column densities at the SO peak of L134N and the NH3 peak of TMC 1 are found to be about 2.6 X 10 to the 13th/sq cm and 7.0 X 10 to the 12th/sq cm, respectively. The results suggest that grain surface reactions may play a major role in the synthesis of H2S in cold, dark clouds.
The published version is located at http://adsabs.harvard.edu/full/1989ApJ...345L..63M
Astrophysics and Astronomy, Extraterrestrial Environment, Astronomy, Spectrum Analysis, DARK MATTER, Astronomical Phenomena, HYDROGEN SULFIDE, ORGANIC COMPOUNDS, INTERSTELLAR GAS, LINE SPECTRA, Interstellar Chemistry, MOLECULAR CLOUDS, ABUNDANCE, ASTRONOMICAL SPECTROSCOPY, Gases, Hydrogen Sulfide
Astrophysics and Astronomy, Extraterrestrial Environment, Astronomy, Spectrum Analysis, DARK MATTER, Astronomical Phenomena, HYDROGEN SULFIDE, ORGANIC COMPOUNDS, INTERSTELLAR GAS, LINE SPECTRA, Interstellar Chemistry, MOLECULAR CLOUDS, ABUNDANCE, ASTRONOMICAL SPECTROSCOPY, Gases, Hydrogen Sulfide
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