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molecules:ism:c4h [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:c4h [2019/10/23 16:57] (current) – mueller | ||
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The butadiynyl radical in its < | The butadiynyl radical in its < | ||
M. Guélin, S. Green, and P. Thaddeus,\\ | M. Guélin, S. Green, and P. Thaddeus,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
before it was actually detected in the laboratory. Two rotational transitions had been reported previously as U-lines in two different publications. The highest frequency fine structure component seems to be overlapped. | before it was actually detected in the laboratory. Two rotational transitions had been reported previously as U-lines in two different publications. The highest frequency fine structure component seems to be overlapped. | ||
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Soon thereafter, it was detected with the OSO 20 m telescope toward TMC-1 by:\\ | Soon thereafter, it was detected with the OSO 20 m telescope toward TMC-1 by:\\ | ||
W. M. Irvine, B. Höglund, P. Friberg, J. Askne, and J. Elldér,\\ | W. M. Irvine, B. Höglund, P. Friberg, J. Askne, and J. Elldér,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
Four hyperfine components of the //N// = 3 – 2 transition were detected near 28.55 GHz. | Four hyperfine components of the //N// = 3 – 2 transition were detected near 28.55 GHz. | ||
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The radical was also observed in the diffuse medium by:\\ | The radical was also observed in the diffuse medium by:\\ | ||
M. B. Bell, P. A. Friedman, and H. E. Matthews,\\ | M. B. Bell, P. A. Friedman, and H. E. Matthews,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
Moreover, the molecule was also detected in several PDRs, namely the Horsehead nebula (B 33), IC 63, and in the //ρ// Oph L1688-W cloud interface: | Moreover, the molecule was also detected in several PDRs, namely the Horsehead nebula (B 33), IC 63, and in the //ρ// Oph L1688-W cloud interface: | ||
D. Teyssier, D. Fossé M. Gerin, J. Pety, A. Abergel, and E. Roueff,\\ | D. Teyssier, D. Fossé M. Gerin, J. Pety, A. Abergel, and E. Roueff,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
Vibrationally excited C< | Vibrationally excited C< | ||
M. Guélin, J. Cernicharo, S. Navarro, D. R. Woodward, C. A. Gottlieb, and P. Thaddeus,\\ | M. Guélin, J. Cernicharo, S. Navarro, D. R. Woodward, C. A. Gottlieb, and P. Thaddeus,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
Subsequent laboratory work revealed these transitions to be due to the // | Subsequent laboratory work revealed these transitions to be due to the // | ||
S. Yamamoto, S. Saito, M. Guélin, J. Cernicharo, H. Suzuki, and M. Ohishi,\\ | S. Yamamoto, S. Saito, M. Guélin, J. Cernicharo, H. Suzuki, and M. Ohishi,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
Unfortunately, | Unfortunately, | ||
Line 35: | Line 35: | ||
C< | C< | ||
B. E. Turner,\\ | B. E. Turner,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The detection of the < | The detection of the < | ||
J. Cernicharo, M. Guélin, and C. Kahane,\\ | J. Cernicharo, M. Guélin, and C. Kahane,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys. Suppl. Ser.// **142** 181–215 (2000). | //Astron. Astrophys. Suppl. Ser.// **142** 181–215 (2000). | ||
Line 47: | Line 47: | ||
Contributor(s): | Contributor(s): | ||
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