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molecules:ism:nccnh-plus [2019/02/27 12:26] – external edit 127.0.0.1 | molecules:ism:nccnh-plus [2022/12/27 13:47] (current) – mueller | ||
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- | ===== On the Detection of Protonated Cyanogen, NCCNH+, in Space ===== | + | ===== On the Detection of Protonated Cyanogen, NCCNH<sup>+</ |
M. Agúndez, J. Cernicharo, P. de Vicente, N. Marcelino, E. Roueff, A. Fuente, M. Gerin, M. Guélin, C. Albo, A. Barcia, L. Barbas, R. Bolaño, F. Colomer, M. C. Diez, J. D. Gallego, J. Gómez-González, | M. Agúndez, J. Cernicharo, P. de Vicente, N. Marcelino, E. Roueff, A. Fuente, M. Gerin, M. Guélin, C. Albo, A. Barcia, L. Barbas, R. Bolaño, F. Colomer, M. C. Diez, J. D. Gallego, J. Gómez-González, | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The //J// = 10 – 9 and 5 – 4 transitions near 88.8 and 44.4 GHz were detected in emission toward the dark cloud TMC-1 (cyanopolyyne peak) and the young stellar object IRAS 18148–0440 in the L483 dense core. The former transition was observed with the IRAM 30 m telescope, the latter with the Yebes 40 m telescope. | The //J// = 10 – 9 and 5 – 4 transitions near 88.8 and 44.4 GHz were detected in emission toward the dark cloud TMC-1 (cyanopolyyne peak) and the young stellar object IRAS 18148–0440 in the L483 dense core. The former transition was observed with the IRAM 30 m telescope, the latter with the Yebes 40 m telescope. | ||
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V. M. Rivilla, J. Martín-Pintado, | V. M. Rivilla, J. Martín-Pintado, | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Mon. Not. R. Soc. Astron.// **483**, L114–L119 (2019).\\ | //Mon. Not. R. Soc. Astron.// **483**, L114–L119 (2019).\\ | ||
The authors also detected HNCCN< | The authors also detected HNCCN< | ||
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Contributor(s): | Contributor(s): | ||
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