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| molecules:ism:h2s [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:h2s [2019/10/21 17:30] (current) – mueller |
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| Hydrogen sulfide has been detected in seven star-forming regions very early as a very abundant molecule via its 1<sub>10</sub> – 1<sub>01</sub> transition in the 2 mm region:\\ | Hydrogen sulfide has been detected in seven star-forming regions very early as a very abundant molecule via its 1<sub>10</sub> – 1<sub>01</sub> transition in the 2 mm region:\\ |
| P. Thaddeus, M. L. Kutner, A. A. Penzias, R. W. Wilson, and K. B. Jefferts,\\ | P. Thaddeus, M. L. Kutner, A. A. Penzias, R. W. Wilson, and K. B. Jefferts,\\ |
| **[[http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1972ApJ...176L..73T|Interstellar Hydrogen Sulfide]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1972ApJ...176L..73T|Interstellar Hydrogen Sulfide]]**\\ |
| //Astrophys. J.// **176**, L73–L76 (1972).\\ | //Astrophys. J.// **176**, L73–L76 (1972).\\ |
| H<sub>2</sub>S was also identified in this transition toward the circumstellar envelope of OH231.8+4.2:\\ | H<sub>2</sub>S was also identified in this transition toward the circumstellar envelope of OH231.8+4.2:\\ |
| N. Ukita, M. Morris,\\ | N. Ukita, M. Morris,\\ |
| **[[http://adsabs.harvard.edu/abs/1983A%26A...121...15U|Hydrogen Sulfide in a Circumstellar Envelope]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1983A%26A...121...15U|Hydrogen Sulfide in a Circumstellar Envelope]]**\\ |
| //Astron Astrophys.// **121**, 15–18 (1983);\\ | //Astron Astrophys.// **121**, 15–18 (1983);\\ |
| and also in certain regions of the cold dark clouds L134N and TMC-1:\\ | and also in certain regions of the cold dark clouds L134N and TMC-1:\\ |
| Y. C. Minh, W. M. Irvine, and L. M. Ziurys,\\ | Y. C. Minh, W. M. Irvine, and L. M. Ziurys,\\ |
| **[[http://dx.doi.org/10.1086/185553|Detection of Interstellar Hydrogen Sulfide in Cold, Dark Clouds]]**\\ | **[[https://doi.org/10.1086/185553|Detection of Interstellar Hydrogen Sulfide in Cold, Dark Clouds]]**\\ |
| //Astrophys. J.// **345**, L63–L66 (1989). | //Astrophys. J.// **345**, L63–L66 (1989). |
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| The same transition was used to identify H<sub>2</sub><sup>34</sup>S toward certain regions in the Orion molecular cloud:\\ | The same transition was used to identify H<sub>2</sub><sup>34</sup>S toward certain regions in the Orion molecular cloud:\\ |
| Y. C. Minh, W. M. Irvine, D. McGonagle, and L. M. Ziurys,\\ | Y. C. Minh, W. M. Irvine, D. McGonagle, and L. M. Ziurys,\\ |
| **[[http://dx.doi.org/10.1086/169103|Observations of the H<sub>2</sub>S toward OMC-1]]**\\ | **[[https://doi.org/10.1086/169103|Observations of the H<sub>2</sub>S toward OMC-1]]**\\ |
| //Astrophys. J.// **360**, 136–141 (1990). | //Astrophys. J.// **360**, 136–141 (1990). |
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| A weak feature near 333 GHz has been identified as the 2<sub>02</sub> – 1<sub>11</sub> of HDS:\\ | A weak feature near 333 GHz has been identified as the 2<sub>02</sub> – 1<sub>11</sub> of HDS:\\ |
| G. H. Macdonald, A. G. Gibb, R. J. Habing, and T. J. Millar,\\ | G. H. Macdonald, A. G. Gibb, R. J. Habing, and T. J. Millar,\\ |
| **[[http://dx.doi.org/10.1051/aas:1996249|A 330–360 GHz Spectral Survey of G 34.3+0.15. I. Data and Physical Analysis]]**\\ | **[[https://doi.org/10.1051/aas:1996249|A 330–360 GHz Spectral Survey of G 34.3+0.15. I. Data and Physical Analysis]]**\\ |
| //Astron Astrophys. Suppl. Ser.// **119**, 333–367 (1996). | //Astron Astrophys. Suppl. Ser.// **119**, 333–367 (1996). |
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| Even D<sub>2</sub>S was recently detected toward two dense, cold clouds Barnard 1 and NGC 1333 IRAS 4A(DCO<sup>+</sup>), with HDS detected toward several additional sources:\\ | Even D<sub>2</sub>S was recently detected toward two dense, cold clouds Barnard 1 and NGC 1333 IRAS 4A(DCO<sup>+</sup>), with HDS detected toward several additional sources:\\ |
| C. Vastel, T. G. Phillips, C. Ceccarelli, and J. C. Pearson,\\ | C. Vastel, T. G. Phillips, C. Ceccarelli, and J. C. Pearson,\\ |
| **[[http://dx.doi.org/10.1086/378261|First Detection of Doubly Deuterated Hydrogen Sulfide]]**\\ | **[[https://doi.org/10.1086/378261|First Detection of Doubly Deuterated Hydrogen Sulfide]]**\\ |
| //Astrophys. J.// **593**, L97–L100 (2003). | //Astrophys. J.// **593**, L97–L100 (2003). |
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| Contributor(s): H. S. P. Müller; 10, 2008; 08, 2018 | Contributor(s): H. S. P. Müller; 10, 2008; 08, 2018 |
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