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molecules:ism:hnc3 [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:hnc3 [2024/04/08 17:56] – mueller | ||
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K. Kawaguchi, S. Takano, M. Ohishi, S.-I. Ishikawa, K. Miyazawa, N. Kaifu, K. Yamashita, S. Yamamoto, S. Saito, Y. Ohshima, and Y. Endo\\ | K. Kawaguchi, S. Takano, M. Ohishi, S.-I. Ishikawa, K. Miyazawa, N. Kaifu, K. Yamashita, S. Yamamoto, S. Saito, Y. Ohshima, and Y. Endo\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
- | The Nobeyama 45 m telescope was used to detect the //J// = 3 – 2, 4 – 3, and 5 – 4 transitions near 28.0, 37.3, and 46.7 GHz. The [[http:// | + | The Nobeyama 45 m telescope was used to detect the //J// = 3 – 2, 4 – 3, and 5 – 4 transitions near 28.0, 37.3, and 46.7 GHz. The [[http:// |
+ | \\ | ||
P. D. Gensheimer reported on\\ | P. D. Gensheimer reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
- | The NRAO 12 m telescope was used to detect the //J// = 11 – 10 transition near 102.7 GHz. The HCCNC to HNC< | + | The NRAO 12 m telescope was used to detect the //J// = 11 – 10 transition near 102.7 GHz. The HCCNC to HNC< |
+ | \\ | ||
C. Vastel, K. Kawaguchi, D. Quénard, M. Ohishi, B. Lefloch, R. Bachiller, and H. S. P. Müller\\ | C. Vastel, K. Kawaguchi, D. Quénard, M. Ohishi, B. Lefloch, R. Bachiller, and H. S. P. Müller\\ | ||
Line 16: | Line 18: | ||
**[[https:// | **[[https:// | ||
//Mon. Not. R. Astron. Soc.// **474**, L76 (2018).\\ | //Mon. Not. R. Astron. Soc.// **474**, L76 (2018).\\ | ||
- | The //J// = 8 – 7, 9 – 8, and 10 – 9 transitions were detected near 74.7, 84.0, and 93.4 GHz. The column density is only slightly smaller than that in TMC-1, similar to HCCNC, even though HC< | + | The //J// = 8 – 7, 9 – 8, and 10 – 9 transitions were detected near 74.7, 84.0, and 93.4 GHz. The column density is only slightly smaller than that in TMC-1, similar to HCCNC, even though HC< |
+ | \\ | ||
+ | J. Cernicharo, N. Marcelino, M. Agúndez, C. Bermúdez, C. Cabezas, B. Tercero, and J. R. Pardo\\ | ||
+ | reported on the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | The authors report the detection of DNC< | ||
+ | \\ | ||
- | ---- | + | J. Cernicharo, B. Tercero, C. Cabezas, M. Agúndez, E. Roueff, R. Fuentetaja, N. Marcelino, and P. de Vicente\\ |
+ | carried out more recently a\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | They reported in the framework of improved data of the above survey the detection of the three HNC< | ||
- | Contributor(s): | ||
+ | ---- | ||
+ | |||
+ | Contributor(s): | ||
---- | ---- | ||