===== Detections of Sulfur Dioxide, SO2, in Space ===== L. E. Snyder, J. M. Hollis, B. L. Ulich, F. J. Lovas, D. R. Johnson, and D. Buhl\\ reported on the\\ **[[http://cdsads.u-strasbg.fr/abs/1975ApJ...198L..81S|Radio Detection of Interstellar Sulfur Dioxide]]**\\ //Astrophys. J.// **198**, L81–L84 (1975).\\ The NRAO 11 m dish was used to detect three transition in the Orion Molecular Cloud-1: 8_1,7 – 8_0,8 (83688.093 MHz); 8_3,5 – 9_2,8 (86639.088 MHz); and 7_3,5 – 8_2,6 (97702.334 MHz). F. P. Schloerb, P. Friberg, Å. Hjalmarson, B. Höglund, and W. M. Irvine\\ reported on\\ **[[http://cdsads.u-strasbg.fr/abs/1983ApJ...264..161S|Observations of Sulfur Dioxide in the Kleinmann-Low Nebula]]**\\ //Astrophys. J.// **284**, 161 – 171 (1983).\\ The OSO 20 m dish was used to detect several transitions of SO₂ along with three of ³⁴SO₂. W. M. Irvine, J. C. Good, and F. P. Schloerb\\ reported on\\ **[[http://cdsads.u-strasbg.fr/abs/1983A&A...127L..10I|Observations of SO₂ and HCS⁺ in Cold Molecular Clouds]]**\\ //Astron. Astrophys.// **127**, L10 – L13 (1983).\\ The FCRAO 14 m dish was used to detect the SO₂ 3_1,3 – 2_0,2 transition near 104029.42 MHz toward the L183 dark cloud. ---- Contributor(s): H. S. P. Müller; 07, 2017 ----