DETECTION OF INTERSTELLAR HYDROGEN-SULFIDE IN COLD, DARK CLOUDS
Publication Date
1989
Journal or Book Title
ASTROPHYSICAL JOURNAL
Abstract
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.
DOI
https://doi.org/10.1086/185553
Pages
L63-L66
Volume
345
Issue
1
Recommended Citation
MINH, YC; Irvine, William M.; and ZIURYS, LM, "DETECTION OF INTERSTELLAR HYDROGEN-SULFIDE IN COLD, DARK CLOUDS" (1989). ASTROPHYSICAL JOURNAL. 252.
https://doi.org/10.1086/185553
Comments
The published version is located at http://adsabs.harvard.edu/full/1989ApJ...345L..63M