molecules:ism:sis

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molecules:ism:sis [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:sis [2019/10/18 12:58] (current) – mueller
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 Silicon monosulfide, SiS, is a very abundant molecule in the inner regions of the circumstellar envelop of IRC+10216 (CW Leo) where it is thought to be the progenitor of much of the Si-chemistry. It was reported first by\\ Silicon monosulfide, SiS, is a very abundant molecule in the inner regions of the circumstellar envelop of IRC+10216 (CW Leo) where it is thought to be the progenitor of much of the Si-chemistry. It was reported first by\\
 M. Morris, W. Gilmore, P. Palmer, B. E. Turner, and B. Zuckerman,\\ M. Morris, W. Gilmore, P. Palmer, B. E. Turner, and B. Zuckerman,\\
-**[[http://cdsads.u-strasbg.fr/abs/1975ApJ...199L..47M|Detection of Interstellar SiS and a Study of the IRC +10216 Molecular Envelope]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1975ApJ...199L..47M|Detection of Interstellar SiS and a Study of the IRC +10216 Molecular Envelope]]**\\
 //Astrophys. J.// **199**, L47–L51 (1975).\\ //Astrophys. J.// **199**, L47–L51 (1975).\\
 The 11 m Kitt Peak telescope was used to detect the //J// = 6 – 5 and 5 – 4 transitions near 108.9 and 90.8 GHz, respectively. The 11 m Kitt Peak telescope was used to detect the //J// = 6 – 5 and 5 – 4 transitions near 108.9 and 90.8 GHz, respectively.
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 D. F. Dickinson and E. N. Rodriguez Kuiper\\ D. F. Dickinson and E. N. Rodriguez Kuiper\\
 reported on\\ reported on\\
-**[[http://cdsads.u-strasbg.fr/abs/1981ApJ...247..112D|Interstellar silicon sulfide]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1981ApJ...247..112D|Interstellar silicon sulfide]]**\\
 //Astrophys. J.// **247**, 112–115 (1981).\\ //Astrophys. J.// **247**, 112–115 (1981).\\
 The same transitions as above were detected toward Sgr B2, and the 6 – 5 transition was detected toward Orion A. The same transitions as above were detected toward Sgr B2, and the 6 – 5 transition was detected toward Orion A.
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 A total of seven rare isotopic species has been detected since. These involve <sup>29</sup>SiS and Si<sup>34</sup>S:\\ A total of seven rare isotopic species has been detected since. These involve <sup>29</sup>SiS and Si<sup>34</sup>S:\\
 L. E. B. Johansson, C. Andersson, J. Ellder, P. Friberg, Å. Hjalmarson, B. Höglund, W. M. Irvine, H. Olofsson, and G. Rydbeck,\\ L. E. B. Johansson, C. Andersson, J. Ellder, P. Friberg, Å. Hjalmarson, B. Höglund, W. M. Irvine, H. Olofsson, and G. Rydbeck,\\
-**[[http://cdsads.u-strasbg.fr/abs/1984A%26A...130..227J|Spectral Scan of Orion A and IRC+10216 from 72 to 91 GHz]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1984A%26A...130..227J|Spectral Scan of Orion A and IRC+10216 from 72 to 91 GHz]]**\\
 //Astron. Astrophys.// **130**, 227–256 (1984);\\ //Astron. Astrophys.// **130**, 227–256 (1984);\\
 <sup>30</sup>SiS:\\ <sup>30</sup>SiS:\\
 L. M. Ziurys, D. P. Clemens, R. J. Saykally, M. Colvin, H. F. Schaefer,\\ L. M. Ziurys, D. P. Clemens, R. J. Saykally, M. Colvin, H. F. Schaefer,\\
-**[[http://cdsads.u-strasbg.fr/abs/1984ApJ...281..219Z|A Search for Interstellar Silicon Nitride]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1984ApJ...281..219Z|A Search for Interstellar Silicon Nitride]]**\\
 //Astrophys. J.// **281**, 219–224 (1984);\\ //Astrophys. J.// **281**, 219–224 (1984);\\
 Si<sup>33</sup>S:\\ Si<sup>33</sup>S:\\
 C. Kahane, J. Gomez-Gonzalez, J. Cernicharo, and M. Guélin,\\ C. Kahane, J. Gomez-Gonzalez, J. Cernicharo, and M. Guélin,\\
-**[[http://cdsads.u-strasbg.fr/abs/1988A%26A...190..167K|Carbon, Nitrogen, Sulfur and Silicon Isotopic Ratios in the Envelope of IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1988A%26A...190..167K|Carbon, Nitrogen, Sulfur and Silicon Isotopic Ratios in the Envelope of IRC +10216]]**\\
 //Astron. Astrophys.// **190**, 167–177 (1988);\\ //Astron. Astrophys.// **190**, 167–177 (1988);\\
 <sup>29</sup>Si<sup>34</sup>S and <sup>30</sup>Si<sup>34</sup>S:\\ <sup>29</sup>Si<sup>34</sup>S and <sup>30</sup>Si<sup>34</sup>S:\\
 J. Cernicharo, M. Guélin, and C. Kahane,\\ J. Cernicharo, M. Guélin, and C. Kahane,\\
-**[[http://cdsads.u-strasbg.fr/abs/2000A%26AS..142..181C|A λ 2 mm Molecular Line Survey of the C-Star Envelope IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/2000A%26AS..142..181C|A λ 2 mm Molecular Line Survey of the C-Star Envelope IRC +10216]]**\\
 //Astron. Astrophys. Suppl.// **142**, 181–215 (2000);\\ //Astron. Astrophys. Suppl.// **142**, 181–215 (2000);\\
 and Si<sup>36</sup>S:\\ and Si<sup>36</sup>S:\\
 R. Mauersberger, U. Ott, C. Henkel, J. Cernicharo, and R. Gallino,\\ R. Mauersberger, U. Ott, C. Henkel, J. Cernicharo, and R. Gallino,\\
-**[[http://dx.doi.org/10.1051/0004-6361:20040451|The Abundance of <sup>36</sup>S in IRC +10216 and its Production in the Galaxy]]**\\+**[[https://doi.org/10.1051/0004-6361:20040451|The Abundance of <sup>36</sup>S in IRC +10216 and its Production in the Galaxy]]**\\
 //Astron. Astrophys.// **426**, 219–227 (2004).\\ //Astron. Astrophys.// **426**, 219–227 (2004).\\
  
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 Maser activity in //v// = 0 of the main isotopic species has been reported first by\\ Maser activity in //v// = 0 of the main isotopic species has been reported first by\\
 C. Henkel, H. E. Matthews, and M. Morris,\\ C. Henkel, H. E. Matthews, and M. Morris,\\
-**[[http://cdsads.u-strasbg.fr/abs/1983ApJ...267..184H|SiS Maser Emission from IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1983ApJ...267..184H|SiS Maser Emission from IRC +10216]]**\\
 //Astrophys. J.// **267**, 184–190 (1983).\\ //Astrophys. J.// **267**, 184–190 (1983).\\
 J. P. Fonfría Expósito, M. Agúndez, B. Tercero, J. R. Pardo, and J. Cernicharo\\ J. P. Fonfría Expósito, M. Agúndez, B. Tercero, J. R. Pardo, and J. Cernicharo\\
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 Vibrationally excited SiS has been detected by\\ Vibrationally excited SiS has been detected by\\
 B. E. Turner,\\ B. E. Turner,\\
-**[[http://cdsads.u-strasbg.fr/abs/1987A%26A...183L..23T|Detection of Vibrationally Excited SiS in IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1987A%26A...183L..23T|Detection of Vibrationally Excited SiS in IRC +10216]]**\\
 //Astron. Astrophys.// **183**, L23–L26 (1987).\\ //Astron. Astrophys.// **183**, L23–L26 (1987).\\
 L. Velilla Prieto, J. Cernicharo, G. Quintana-Lacaci, M. Agúndez, A. Castro-Carrizo, J. P. Fonfría, N. Marcelino, J. Zúñiga, A. Requena, and A. Bastida\\ L. Velilla Prieto, J. Cernicharo, G. Quintana-Lacaci, M. Agúndez, A. Castro-Carrizo, J. P. Fonfría, N. Marcelino, J. Zúñiga, A. Requena, and A. Bastida\\
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 Rovibrational transitions were observed by\\ Rovibrational transitions were observed by\\
 R. J. Boyle, J. J. Keady, D. E. Jennings, K. L. Hirsch, and G. R. Wiedemann,\\ R. J. Boyle, J. J. Keady, D. E. Jennings, K. L. Hirsch, and G. R. Wiedemann,\\
-**[[http://cdsads.u-strasbg.fr/abs/1994ApJ...420..863B|Observations of 13.5 micron Rotation-Vibration Lines of SiS in IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1994ApJ...420..863B|Observations of 13.5 micron Rotation-Vibration Lines of SiS in IRC +10216]]**\\
 //Astrophys. J.// **420**, 863–868 (1994). //Astrophys. J.// **420**, 863–868 (1994).
  
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 Contributor(s): H. S. P. Müller, 02, 2007; 06, 2008; 07, 2017; 12, 2017. Contributor(s): H. S. P. Müller, 02, 2007; 06, 2008; 07, 2017; 12, 2017.
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