OBSERVATIONS OF H2S TOWARD OMC-1
Journal or Book Title
Observations of the 1(10) - 1(01) transition of interstellar H2S and its isotopes toward OMC-1 are reported. The fractional abundance of H2S in the quiescent regions of OMC-1 seems difficult to explain by currently known ion-molecular reactions. The fractional abundance of H2S relative to H2 is enhanced by a factor of 1000 in the hot core and the plateau relative to the quiescent clouds. The (HDS)/(H2S) abundance ratio in the hot core is estimated at 0.02 or less.
MINH, YC; ZIURYS, LM; Irvine, William M.; and MCGONAGLE, D, "OBSERVATIONS OF H2S TOWARD OMC-1" (1990). ASTROPHYSICAL JOURNAL. 245.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/245