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| molecules:ism:mecn [2019/10/23 21:59] – mueller | molecules:ism:mecn [2025/09/03 14:46] (current) – mueller |
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| both <sup>13</sup>C species were detected by\\ | both <sup>13</sup>C species were detected by\\ |
| E. C. Sutton, G. A. Blake, C. R. Masson, and T. G. Phillips,\\ | E. C. Sutton, G. A. Blake, C. R. Masson, and T. G. Phillips,\\ |
| **[[http://cdsads.u-strasbg.fr/abs/1985ApJS...58..341S|Molecular Line Survey of Orion A from 215 to 247 GHz]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1985ApJS...58..341S|Molecular Line Survey of Orion A from 215 to 247 GHz]]**\\ |
| //Astrophys. J. Suppl. Ser.// **58**, 341–378 (1985). | //Astrophys. J. Suppl. Ser.// **58**, 341–378 (1985). |
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| //Astrophys. J.// **274**, 184–194 (1983). | //Astrophys. J.// **274**, 184–194 (1983). |
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| S. M. Fortman, J. P. McMillan, C. F.Neese, S. K. Randall, A. J. Remijan, T. L. Wilson, and F. C. De Lucia\\ | S. M. Fortman, J. P. McMillan, C. F. Neese, S. K. Randall, A. J. Remijan, T. L. Wilson, and F. C. De Lucia\\ |
| gave a brief account on the detection of //v//<sub>8</sub> = 2 in their work\\ | gave a brief account on the detection of //v//<sub>8</sub> = 2 in their work\\ |
| **[[https://doi.org/10.1016/j.jms.2012.08.002|An analysis of a preliminary ALMA Orion KL spectrum via the use of complete experimental spectra from the laboratory]]**\\ | **[[https://doi.org/10.1016/j.jms.2012.08.002|An analysis of a preliminary ALMA Orion KL spectrum via the use of complete experimental spectra from the laboratory]]**\\ |
| **[[https://doi.org/10.1051/0004-6361/201321096|Complex Organic Molecules in the Interstellar Medium: IRAM 30 m Line Survey of Sagittarius B2(N) and (M)]]**\\ | **[[https://doi.org/10.1051/0004-6361/201321096|Complex Organic Molecules in the Interstellar Medium: IRAM 30 m Line Survey of Sagittarius B2(N) and (M)]]**\\ |
| //Astron. Astrophys.// **559**, Art. No. A47 (2013).\\ | //Astron. Astrophys.// **559**, Art. No. A47 (2013).\\ |
| Besides observing these two lower lying vibrational states, they detected transitions pertaining to //v//<sub>4</sub> = 1, the next higher state, as well as transitions of the <sup>13</sup>C isotopologs in their //v//<sub>8</sub> = 1 vibrational states. | Besides observing these two lower lying vibrational states, they detected transitions pertaining to //v//<sub>4</sub> = 1, the next higher state, as well as transitions of the <sup>13</sup>C isotopologs in their //v//<sub>8</sub> = 1 vibrational states.\\ |
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