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--- molecules:ism:ch3oh [2022/04/29 13:46] – mueller
+++ molecules:ism:ch3oh [2022/04/29 13:56] (current) – mueller
@@ Line 72: / Line 72: @@
 V. V. Ilyushin, H. S. P. Müller, J. K. Jørgensen, S. Bauerecker, C. Maul, Y. Bakhmat, E. A. Alekseev, O. Dorovskaya, S. Vlasenko, F. Lewen, S. Schlemmer, K. Berezkin, and R. M. Lees\\
 investigated the\\
-**[[https://doi.org/10.1051/0004-6361/202142326|Rotational and rovibrational spectroscopy of CD3OH with an account of CD3OH toward IRAS 16293−2422]]**\\
+**[[https://doi.org/10.1051/0004-6361/202142326|Rotational and Rovibrational Spectroscopy of CD<sub>3</sub>OH with an Account of CD<sub>3</sub>OH toward IRAS 16293−2422]]**\\
-//Astron. Astrophys.// **416**, 159–163 (2004).\\
+//Astron. Astrophys.// **658**, Art. No. A127 (2022).\\
+Using the Protostellar Interferometric Line Survey carried out with ALMA, several lines of torsionally excited CD<sub>3</sub>OH were detected between 329 and 363 GHz; nine unblended or only slightly blended lines of this vibrationally excited state were shown in a figure around 350.6 GHz. The rotational temperature was ~225 K, and the CH<sub>3</sub>OH to CD<sub>3</sub>OH ratio was about 300. Lines of torsionally excited deuterated methanol will be more prominent for <sup>12</sup>C isotopologs containing fewer D atoms.\\
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