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| molecules:ism:l-c3h2 [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:l-c3h2 [2019/10/23 16:58] (current) – mueller |
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| 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..39C|Astronomical Detection of H<sub>2</sub>CCC]]**,\\ | **[[https://ui.adsabs.harvard.edu/abs/1991ApJ...368L..39C|Astronomical Detection of H<sub>2</sub>CCC]]**,\\ |
| //Astrophys. J.// **368**, L39–L41 (1991)\\ | //Astrophys. J.// **368**, L39–L41 (1991)\\ |
| The //para// ground state transition 1<sub>0,1</sub> – 0<sub>0,0</sub> near 20.8 GHz was detected with the Effelsberg 100 m telescope in emission together with the //ortho// transitions 5<sub>1,5</sub> – 4<sub>1,4</sub>, 5<sub>1,4</sub> – 4<sub>1,3</sub>, and 7<sub>1,6</sub> – 6<sub>1,5</sub> near 103.0, 104.9, and 146.9 GHz, respectively. These transitions were made with the IRAM 30 m telescope. The molecule may have been detected also in the circumstellar envelope of CW Leonis, also known as IRC +10216. | The //para// ground state transition 1<sub>0,1</sub> – 0<sub>0,0</sub> near 20.8 GHz was detected with the Effelsberg 100 m telescope in emission together with the //ortho// transitions 5<sub>1,5</sub> – 4<sub>1,4</sub>, 5<sub>1,4</sub> – 4<sub>1,3</sub>, and 7<sub>1,6</sub> – 6<sub>1,5</sub> near 103.0, 104.9, and 146.9 GHz, respectively. These transitions were made with the IRAM 30 m telescope. The molecule may have been detected also in the circumstellar envelope of CW Leonis, also known as IRC +10216. |
| J. Cernicharo, P. Cox, D. Fossé and R. Güsten,\\ | J. Cernicharo, P. Cox, D. Fossé and R. Güsten,\\ |
| reported on the\\ | reported on the\\ |
| **[[http://cdsads.u-strasbg.fr/abs/1999A%26A...351..341C|Detection of Linear C<sub>3</sub>H<sub>2</sub> in Absorption toward Continuum Sources]]**,\\ | **[[https://ui.adsabs.harvard.edu/abs/1999A%26A...351..341C|Detection of Linear C<sub>3</sub>H<sub>2</sub> in Absorption toward Continuum Sources]]**,\\ |
| //Astron. Astrophys.// **351**, 341–346 (1999)\\ | //Astron. Astrophys.// **351**, 341–346 (1999)\\ |
| The 1<sub>0,1</sub> – 0<sub>0,0</sub> transition was observed in absorption toward the continuum sources W49, W51e1/e2 and W51D. | The 1<sub>0,1</sub> – 0<sub>0,0</sub> transition was observed in absorption toward the continuum sources W49, W51e1/e2 and W51D. |
| The Molecule was also deteceted in a source of Warm Carbon Chain Chemistry by\\ | The Molecule was also deteceted in a source of Warm Carbon Chain Chemistry by\\ |
| N. Sakai, T. Sakai, T. Hirota, and S. Yamamoto,\\ | N. Sakai, T. Sakai, T. Hirota, and S. Yamamoto,\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201424568|Abundant Carbon-Chain Molecules toward the Low-Mass Protostar IRAS 04368+2557 in L1527]]**,\\ | **[[https://doi.org/10.1051/0004-6361/201424568|Abundant Carbon-Chain Molecules toward the Low-Mass Protostar IRAS 04368+2557 in L1527]]**,\\ |
| //Astrophys. J.// **672**, 371–381 (2008) | //Astrophys. J.// **672**, 371–381 (2008) |
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| The Molecule was also deteceted in the CO<sup>+</sup> peak of the Orion Bar photodissociation regions by\\ | The Molecule was also deteceted in the CO<sup>+</sup> peak of the Orion Bar photodissociation regions by\\ |
| S. Cuadrado, J. R. Goicoechea, P. Piller, J. Cernicharo, A. Fuente, and C. Joblin,\\ | S. Cuadrado, J. R. Goicoechea, P. Piller, J. Cernicharo, A. Fuente, and C. Joblin,\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201424568|The Chemistry and Spatial Distribution of Small Hydrocarbons in UV-irradiated Molecular Clouds: the Orion Bar PDR]]**,\\ | **[[https://doi.org/10.1051/0004-6361/201424568|The Chemistry and Spatial Distribution of Small Hydrocarbons in UV-irradiated Molecular Clouds: the Orion Bar PDR]]**,\\ |
| //Astron. Astrophys.// **575**, Art. No. A82 (2015) | //Astron. Astrophys.// **575**, Art. No. A82 (2015) |
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| S. Spezzano, H. Gupta, S. Brünken, C. A. Gottlieb, P. Caselli, K. M. Menten, H. S. P. Müller, L. Bizzocchi, P. Schilke, M. C. McCarthy, and S. Schlemmer,\\ | S. Spezzano, H. Gupta, S. Brünken, C. A. Gottlieb, P. Caselli, K. M. Menten, H. S. P. Müller, L. Bizzocchi, P. Schilke, M. C. McCarthy, and S. Schlemmer,\\ |
| reported on the\\ | reported on the\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201527460|A Study of the C<sub>3</sub>H<sub>2</sub> Isomers and Isotopologues: First Interstellar Detection of HDCCC]]**,\\ | **[[https://doi.org/10.1051/0004-6361/201527460|A Study of the C<sub>3</sub>H<sub>2</sub> Isomers and Isotopologues: First Interstellar Detection of HDCCC]]**,\\ |
| //Astron. Astrophys.// **575**, Art. No. A110 (2016)\\ | //Astron. Astrophys.// **575**, Art. No. A110 (2016)\\ |
| The 5<sub>0,5</sub> – 4<sub>0,4</sub> transition near 96.9 GHz was detected with the IRAM 30 m telescope in emission toward the starless cores TMC-1C and L1544. In addition, the 1<sub>0,1</sub> – 0<sub>0,0</sub> transition near 19.4 GHz was detected in TMC-1 with the 100 m GBT. | The 5<sub>0,5</sub> – 4<sub>0,4</sub> transition near 96.9 GHz was detected with the IRAM 30 m telescope in emission toward the starless cores TMC-1C and L1544. In addition, the 1<sub>0,1</sub> – 0<sub>0,0</sub> transition near 19.4 GHz was detected in TMC-1 with the 100 m GBT. |
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| Contributor(s): H. S. P. Müller; 02, 2016 | Contributor(s): H. S. P. Müller; 02, 2016 |
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