molecules:ism:ammoniak

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molecules:ism:ammoniak [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:ammoniak [2019/10/22 16:39] (current) – mueller
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 NH<sub>3</sub> was observed first in its lowest //J// = //K// = 1 tunneling transition toward Sagittarius B2 (Sgr B2):\\ NH<sub>3</sub> was observed first in its lowest //J// = //K// = 1 tunneling transition toward Sagittarius B2 (Sgr B2):\\
 A. C. Cheung, D. M. Rank, C. H. Townes, D. D. Thornton, and W. J. Welch,\\ A. C. Cheung, D. M. Rank, C. H. Townes, D. D. Thornton, and W. J. Welch,\\
-**[[http://dx.doi.org/10.1103/PhysRevLett.21.1701|Detection of NH<sub>3</sub> Molecules in the Interstellar Medium by Their Microwave Emission]]**\\+**[[https://doi.org/10.1103/PhysRevLett.21.1701|Detection of NH<sub>3</sub> Molecules in the Interstellar Medium by Their Microwave Emission]]**\\
 //Phys. Rev. Lett.// **21**, 1701–1705 (1968). //Phys. Rev. Lett.// **21**, 1701–1705 (1968).
  
 NH<sub>2</sub>D was detected initially toward Sgr B2 and Orion KL:\\ NH<sub>2</sub>D was detected initially toward Sgr B2 and Orion KL:\\
 B. E. Turner, B. Zuckerman, M. Morris, and P.Palmer,\\ B. E. Turner, B. Zuckerman, M. Morris, and P.Palmer,\\
-**[[http://cdsads.u-strasbg.fr/abs/1978ApJ...219L..43T|Microwave Detection of Interstellar Deuterated Ammonia]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1978ApJ...219L..43T|Microwave Detection of Interstellar Deuterated Ammonia]]**\\
 //Astrophys. J.// **219**, L43–L47 (1978).\\ //Astrophys. J.// **219**, L43–L47 (1978).\\
 E. N. Rodriguez Kuiper, B. Zuckerman, and T. B. H. Kuiper,\\ E. N. Rodriguez Kuiper, B. Zuckerman, and T. B. H. Kuiper,\\
-**[[http://cdsads.u-strasbg.fr/abs/1978ApJ...219L..49R|Deuterated Ammonia Toward the Orion Nebula]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1978ApJ...219L..49R|Deuterated Ammonia Toward the Orion Nebula]]**\\
 //Astrophys. J.// **219**, L49–L53 (1978). //Astrophys. J.// **219**, L49–L53 (1978).
  
 <sup>15</sup>NH<sub>3</sub> was observed toward the Orion Molecular Cloud (OMC-1) soon thereafter:\\ <sup>15</sup>NH<sub>3</sub> was observed toward the Orion Molecular Cloud (OMC-1) soon thereafter:\\
 T. L. Wilson and T. Pauls,\\ T. L. Wilson and T. Pauls,\\
-**[[http://cdsads.u-strasbg.fr/abs/1979A%26A....73L..10W|The Detection of Interstellar <sup>15</sup>NH<sub>3</sub>]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1979A%26A....73L..10W|The Detection of Interstellar <sup>15</sup>NH<sub>3</sub>]]**\\
 //Astron. Astrophys.// **73**, L10–L12 (1979). //Astron. Astrophys.// **73**, L10–L12 (1979).
  
 The first detection of a rotation-inversion transition of NH<sub>3</sub> was also reported: J. Keene, G. A. Blake, and T. G. Philips,\\ The first detection of a rotation-inversion transition of NH<sub>3</sub> was also reported: J. Keene, G. A. Blake, and T. G. Philips,\\
-**[[http://cdsads.u-strasbg.fr/abs/1983ApJ...271L..27K|First Detection of the Ground-State //J<sub>K</sub>// = 1<sub>0</sub> – 0<sub>0</sub> Submillimeter Transition of Interstellar Ammonia]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1983ApJ...271L..27K|First Detection of the Ground-State //J<sub>K</sub>// = 1<sub>0</sub> – 0<sub>0</sub> Submillimeter Transition of Interstellar Ammonia]]**\\
 //Astrophys. J.// **271**, L27–L30 (1983). //Astrophys. J.// **271**, L27–L30 (1983).
  
 NHD<sub>2</sub> was detected first toward the L134N dark cloud which is also known as L183:\\ NHD<sub>2</sub> was detected first toward the L134N dark cloud which is also known as L183:\\
 E. Roueff, S. Tiné, L. H. Coudert, G. Pineau des Forêts, E. Falgarone, and M. Gerin,\\ E. Roueff, S. Tiné, L. H. Coudert, G. Pineau des Forêts, E. Falgarone, and M. Gerin,\\
-**[[http://cdsads.u-strasbg.fr/abs/2000A%26A...354L..63R|Detection of Doubly Deuterated Ammonia in L134N]]**\\+**[[https://ui.adsabs.harvard.edu/abs/2000A%26A...354L..63R|Detection of Doubly Deuterated Ammonia in L134N]]**\\
 //Astron. Astrophys.// **354**, L63–L66 (2000). //Astron. Astrophys.// **354**, L63–L66 (2000).
  
 Finally, even ND<sub>3</sub> was detected in NGC 1333 and in the Barnard 1 Cloud:\\ Finally, even ND<sub>3</sub> was detected in NGC 1333 and in the Barnard 1 Cloud:\\
 F. F. S. van der Tak, P. Schilke, H. S. P. Müller, D. C. Lis, T. G. Phillips, M. Gerin, and E. Roueff,\\ F. F. S. van der Tak, P. Schilke, H. S. P. Müller, D. C. Lis, T. G. Phillips, M. Gerin, and E. Roueff,\\
-**[[http://dx.doi.org/10.1051/0004-6361:20020647|Triply Deuterated Ammonia in NGC 1333]]**\\+**[[https://doi.org/10.1051/0004-6361:20020647|Triply Deuterated Ammonia in NGC 1333]]**\\
 //Astron. Astrophys.// **388**, L53–L56 (2002).\\ //Astron. Astrophys.// **388**, L53–L56 (2002).\\
 D. C. Lis, E. Roueff, M. Gerin, T. G. Phillips, L. H. Coudert, F. F. S. van der Tak, and P. Schilke,\\ D. C. Lis, E. Roueff, M. Gerin, T. G. Phillips, L. H. Coudert, F. F. S. van der Tak, and P. Schilke,\\
-**[[http://dx.doi.org/10.1086/341132|Detection of Triply Deuterated Ammonia in the Barnard 1 Cloud]]**\\+**[[https://doi.org/10.1086/341132|Detection of Triply Deuterated Ammonia in the Barnard 1 Cloud]]**\\
 //Astrophys. J.// **571**, L55–L58 (2002). //Astrophys. J.// **571**, L55–L58 (2002).
  
 The detection of vibrationally excited NH<sub>3</sub> (//v//<sub>2</sub> = 1) was reported in:\\ The detection of vibrationally excited NH<sub>3</sub> (//v//<sub>2</sub> = 1) was reported in:\\
 R. Mauersberger, C. Henkel, and T. L. Wilson,\\ R. Mauersberger, C. Henkel, and T. L. Wilson,\\
-**[[http://cdsads.u-strasbg.fr/abs/1988A%26A...205..235M|Vibrationally Excited Ammonia toward Orion-KL]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1988A%26A...205..235M|Vibrationally Excited Ammonia toward Orion-KL]]**\\
 //Astron. Astrophys.// **205**, 235–242 (1988). //Astron. Astrophys.// **205**, 235–242 (1988).
  
 The observation of 1<sub>11</sub> (0<sup>+</sup>) – 1<sub>01</sub> (0<sup>–</sup>) //ortho// transition of <sup>15</sup>NH<sub>2</sub>D with the IRAM 30m telescope toward Barnard-1b, NGC1333-DCO<sup>+</sup>, and L1689N was reported by:\\ The observation of 1<sub>11</sub> (0<sup>+</sup>) – 1<sub>01</sub> (0<sup>–</sup>) //ortho// transition of <sup>15</sup>NH<sub>2</sub>D with the IRAM 30m telescope toward Barnard-1b, NGC1333-DCO<sup>+</sup>, and L1689N was reported by:\\
 M. Gerin, N. Marcelino, N. Biver, E. Roueff, L. H. Coudert, M. Elkeurti, D. C. Lis, and D. Bockelée-Morvan,\\ M. Gerin, N. Marcelino, N. Biver, E. Roueff, L. H. Coudert, M. Elkeurti, D. C. Lis, and D. Bockelée-Morvan,\\
-**[[http://dx.doi.org/10.1051/0004-6361/200911759|Detection of <sup>15</sup>NH<sub>2</sub>D in dense cores: a new tool for measuring the <sup>14</sup>N/<sup>15</sup>N ratio in the cold ISM]]**\\+**[[https://doi.org/10.1051/0004-6361/200911759|Detection of <sup>15</sup>NH<sub>2</sub>D in dense cores: a new tool for measuring the <sup>14</sup>N/<sup>15</sup>N ratio in the cold ISM]]**\\
 //Astron. Astrophys.// **498**, L9–L12 (2009). //Astron. Astrophys.// **498**, L9–L12 (2009).
  
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 Contributor(s): H. S. P. Müller; 12, 2004; 06, 2006 & 01, 2010 Contributor(s): H. S. P. Müller; 12, 2004; 06, 2006 & 01, 2010
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