Differences

This shows you the differences between two versions of the page.

--- molecules:ism:mesh [2025/02/24 15:27] – mueller
+++ molecules:ism:mesh [2025/10/29 11:19] (current) – mueller
@@ Line 5: / Line 5: @@
 **[[https://ui.adsabs.harvard.edu/abs/1979ApJ...234L.139L|Interstellar methyl mercaptan]]**\\
 //Astrophys. J.// **232**, L139–L142 (1979).\\
-features belonging to several more //J// = 3 –2 and 4 –3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K.\\
+features belonging to several more //J// = 3 – 2 and 4 – 3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K.\\
 \\
@@ Line 40: / Line 40: @@
 **[[https://doi.org/10.3847/2041-8213/adacea|Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH2DSH)]]**\\
 //Astrophys. J. Lett.// **980**, Art. No. L13 (2025).\\
+The isotopolog was identified in the Protostellar Interferometric Line Survey (PILS) toward the solar-like protostar IRAS 16293−2422 B. Eight lines were detected that were deemed to be unblended or only slightly blended. Several other transitions were covered, but most of them were severely blended. The derived CH<sub>2</sub>DSH to CH<sub>3</sub>SH ratio is about 0.055. An earlier search for CH<sub>3</sub>SD by [[https://doi.org/10.1051/0004-6361/201834472|O. Zhakharenko et al.]], //Astron. Astrophys.// **621**, Art. No. A114 (2019) was unsuccessful and, with respect to the present finding, not particularly constraining.\\
+\\
 ----