molecules:ism:menc

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Last revisionBoth sides next revision
molecules:ism:menc [2023/09/26 10:33] muellermolecules:ism:menc [2023/09/26 10:34] mueller
Line 26: Line 26:
 reported on\\ reported on\\
 [[https://doi.org/10.1051/0004-6361/201833140|The ALMA-PILS survey: First detection of methyl isocyanide (CH<sub>3</sub>NC) in a solar-type protostar]]\\ [[https://doi.org/10.1051/0004-6361/201833140|The ALMA-PILS survey: First detection of methyl isocyanide (CH<sub>3</sub>NC) in a solar-type protostar]]\\
-//Astron. Astrophys.// **** (2018), in press.\\+//Astron. Astrophys.// **617** (2018), Art. No. A95.\\
 Several transitions with //J// = 17 – 16 and 18 – 17 and //K// between 0 and 7 were detected near 342 and 362 GHz, respectively toward source B. The molecule was not detected toward source A. The CH<sub>3</sub>CN to CH<sub>3</sub>NC ratio is about 200 toward source B and more than 5000 toward source A.\\ Several transitions with //J// = 17 – 16 and 18 – 17 and //K// between 0 and 7 were detected near 342 and 362 GHz, respectively toward source B. The molecule was not detected toward source A. The CH<sub>3</sub>CN to CH<sub>3</sub>NC ratio is about 200 toward source B and more than 5000 toward source A.\\
 \\ \\
  • molecules/ism/menc.txt
  • Last modified: 2023/09/26 10:35
  • by mueller