Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== 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<sub>1,7</sub> – 8<sub>0,8</sub> (83688.093 MHz); 8<sub>3,5</sub> – 9<sub>2,8</sub> (86639.088 MHz); and 7<sub>3,5</sub> – 8<sub>2,6</sub> (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 SO<sub>2</sub> along with three of <sup>34</sup>SO<sub>2</sub>. W. M. Irvine, J. C. Good, and F. P. Schloerb\\ reported on\\ **[[http://cdsads.u-strasbg.fr/abs/1983A&A...127L..10I|Observations of SO<sub>2</sub> and HCS<sup>+</sup> in Cold Molecular Clouds]]**\\ //Astron. Astrophys.// **127**, L10 – L13 (1983).\\ The FCRAO 14 m dish was used to detect the SO<sub>2</sub> 3<sub>1,3</sub> – 2<sub>0,2</sub> transition near 104029.42 MHz toward the L183 dark cloud. ---- Contributor(s): H. S. P. Müller; 07, 2017 ---- molecules/ism/so2.txt Last modified: 2019/02/25 22:38by 127.0.0.1