molecules:ism:ns

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molecules:ism:ns [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:ns [2019/10/18 12:53] (current) – mueller
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 The two Λ components of the //J// = 5/2 – 3/2 pertaining to the lower energy Π<sub>1/2</sub> ladder were detected with the NRAO 11 m telescope between 115 and 116 GHz toward Sgr B2(OH) by:\\ The two Λ components of the //J// = 5/2 – 3/2 pertaining to the lower energy Π<sub>1/2</sub> ladder were detected with the NRAO 11 m telescope between 115 and 116 GHz toward Sgr B2(OH) by:\\
 C. A. Gottlieb, J. A. Ball, E. W. Gottlieb, C. J. Lada, and H. Penfield,\\ C. A. Gottlieb, J. A. Ball, E. W. Gottlieb, C. J. Lada, and H. Penfield,\\
-**[[http://cdsads.u-strasbg.fr/abs/1975ApJ...200L.147G|Detection of Interstellar Nitrogen Sulfide]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1975ApJ...200L.147G|Detection of Interstellar Nitrogen Sulfide]]**\\
 //Astrophys. J.// **200**, L147–L149 (1975).\\ //Astrophys. J.// **200**, L147–L149 (1975).\\
 The features displayed partially resolved hyperfine structure. The molecules was also detected in this and other transitions toward several other hot cores. The features displayed partially resolved hyperfine structure. The molecules was also detected in this and other transitions toward several other hot cores.
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 NS was also observed in TMC-1 and L134 by:\\ NS was also observed in TMC-1 and L134 by:\\
 D. McGonagle, W. M. Irvine, and M. Ohishi,\\ D. McGonagle, W. M. Irvine, and M. Ohishi,\\
-**[[http://cdsads.u-strasbg.fr/abs/1994ApJ...422..621M|Nitrogen Sulfide in Quiescent Dark Clouds]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1994ApJ...422..621M|Nitrogen Sulfide in Quiescent Dark Clouds]]**\\
 //Astrophys. J.// **422**, 621–625 (1994). //Astrophys. J.// **422**, 621–625 (1994).
  
 It has been detected in a planetary nebula:\\ It has been detected in a planetary nebula:\\
 C. Sánchez Contreras, V. Bujarrabal, R. Neri, and J. Alcolea,\\ C. Sánchez Contreras, V. Bujarrabal, R. Neri, and J. Alcolea,\\
-**[[http://adsabs.harvard.edu/abs/2000A%26A...357..651S|High-resolution observations at λ = 3 mm of the OH231.8+4.2 molecular outflow]]**\\+**[[https://ui.adsabs.harvard.edu/abs/2000A%26A...357..651S|High-resolution observations at λ = 3 mm of the OH231.8+4.2 molecular outflow]]**\\
 //Astron. Astrophys.// **357**, 651–660 (2000). //Astron. Astrophys.// **357**, 651–660 (2000).
  
 NS occurs in PDRs as well:\\ NS occurs in PDRs as well:\\
 S. Leurini, R. Rolffs, S. Thorwirth, B. Parise, P. Schilke, C. Comito, F. Wyrowski, R. Güsten, P. Bergman, K. M. Menten, and L.-Å. Nyman,\\ S. Leurini, R. Rolffs, S. Thorwirth, B. Parise, P. Schilke, C. Comito, F. Wyrowski, R. Güsten, P. Bergman, K. M. Menten, and L.-Å. Nyman,\\
-**[[http://dx.doi.org/10.1051/0004-6361:20065555|APEX 1 mm Line Survey of the Orion Bar]]**\\+**[[https://doi.org/10.1051/0004-6361:20065555|APEX 1 mm Line Survey of the Orion Bar]]**\\
 //Astron. Astrophys.// **454**, L47–L50 (2006). //Astron. Astrophys.// **454**, L47–L50 (2006).
  
 N<sup>34</sup>S has been identified tentative in Sgr B2(OH) by:\\ N<sup>34</sup>S has been identified tentative in Sgr B2(OH) by:\\
 B. E. Turner,\\ B. E. Turner,\\
-**[[http://cdsads.u-strasbg.fr/abs/1989ApJS...70..539T|A molecular line survey of Sagittarius B2 and Orion-KL from 70 to 115 GHz. I - The observational data]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1989ApJS...70..539T|A molecular line survey of Sagittarius B2 and Orion-KL from 70 to 115 GHz. I - The observational data]]**\\
 //Astrophys. J. Suppl. Ser.// **70**, 539–622 (1989). //Astrophys. J. Suppl. Ser.// **70**, 539–622 (1989).
  
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