molecules:ism:l-c4h2

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision		 Previous revision
molecules:ism:l-c4h2 [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:l-c4h2 [2019/10/23 21:58] (current) – mueller
Line 4: Line 4:
 J. Cernicharo, C. A. Gottlieb, M Guélin, T. C. Killian, G. Paubert, P. Thaddeus, and J. M. Vrtilek,\\ J. Cernicharo, C. A. Gottlieb, M Guélin, T. C. Killian, G. Paubert, P. Thaddeus, and J. M. Vrtilek,\\
 reported on the\\ reported on the\\
-**[[http://cdsads.u-strasbg.fr/abs/1991ApJ...368L..43C|Astronomical Detection of H<sub>2</sub>CCCC]]**,\\+**[[https://ui.adsabs.harvard.edu/abs/1991ApJ...368L..43C|Astronomical Detection of H<sub>2</sub>CCCC]]**,\\
 //Astrophys. J.// **368**, L43–L45 (1991)\\ //Astrophys. J.// **368**, L43–L45 (1991)\\
 The molecule was detectedin the circumstellar envelope of CW Leonis, also known as IRC +10216 using the IRAM 30 m telescope. 10 transitions with 9 ≤ //J'// ≤ 16 were sought, and 8 were detected, two of them partially blended. Six transitions had //K<sub>a</sub>// = 1 (//ortho//) and two had //K<sub>a</sub>// = 0 (//para//). The molecule was detectedin the circumstellar envelope of CW Leonis, also known as IRC +10216 using the IRAM 30 m telescope. 10 transitions with 9 ≤ //J'// ≤ 16 were sought, and 8 were detected, two of them partially blended. Six transitions had //K<sub>a</sub>// = 1 (//ortho//) and two had //K<sub>a</sub>// = 0 (//para//).
Line 10: Line 10:
 The Molecule was also deteceted in the dark cloud TMC-1 by\\ The Molecule was also deteceted in the dark cloud TMC-1 by\\
 K. Kawaguchi, N. Kaifu, M. Ohishi, S.-I. Ishikawa, Y. Hirahara, S. Yamamoto, S. Saito, S. Takano, A. Murakami, J. M. Vrtilek, C. A. Gottlieb, P. Thaddeus, and W. M. Irvine,\\ K. Kawaguchi, N. Kaifu, M. Ohishi, S.-I. Ishikawa, Y. Hirahara, S. Yamamoto, S. Saito, S. Takano, A. Murakami, J. M. Vrtilek, C. A. Gottlieb, P. Thaddeus, and W. M. Irvine,\\
-**[[http://cdsads.u-strasbg.fr/abs/1991PASJ...43..607K|Observations of Cumulene Carbenes, H<sub>2</sub>CCCC and H<sub>2</sub>CCC, in TMC-1]]**,\\+**[[https://ui.adsabs.harvard.edu/abs/1991PASJ...43..607K|Observations of Cumulene Carbenes, H<sub>2</sub>CCCC and H<sub>2</sub>CCC, in TMC-1]]**,\\
 //Publs. Astron. Soc. Japan// **43**, 607–619 (1991) //Publs. Astron. Soc. Japan// **43**, 607–619 (1991)
  
 N. Sakai, T. Sakai, T. Hirota, and S. Yamamoto,\\ N. Sakai, T. Sakai, T. Hirota, and S. Yamamoto,\\
 reported on\\ reported on\\
-**[[http://dx.doi.org/10.1088/0004-637X/702/2/1025|Deuterated Molecules in Warm Carbon Chain Chemsitry: The L1527 Case]]**,\\+**[[https://doi.org/10.1088/0004-637X/702/2/1025|Deuterated Molecules in Warm Carbon Chain Chemsitry: The L1527 Case]]**,\\
 //Astrophys. J.// **702**, 1025–1035 (2009)\\ //Astrophys. J.// **702**, 1025–1035 (2009)\\
 The 5<sub>0,5</sub> – 4<sub>0,4</sub> transition of //l//-C<sub>4</sub>HD near 42.4 GHz was detected with the Nobeyama 45 m telescope in emission. The 5<sub>0,5</sub> – 4<sub>0,4</sub> transition of //l//-C<sub>4</sub>HD near 42.4 GHz was detected with the Nobeyama 45 m telescope in emission.
Line 23: Line 23:
  
 Contributor(s): H. S. P. Müller; 02, 2016 Contributor(s): H. S. P. Müller; 02, 2016
- 
  
 ---- ----
  
  
  • molecules/ism/l-c4h2.1551130726.txt.gz
  • Last modified: 2019/02/25 22:38
  • by 127.0.0.1