molecules:ism:oh

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
molecules:ism:oh [2026/07/29 11:40] – muellermolecules:ism:oh [2026/07/29 11:43] (current) – mueller
Line 95: Line 95:
 **[[https://doi.org/10.1051/0004-6361/201218784|Detection of OD towards the Low-Mass Protostar IRAS 16293−2422]]**\\ **[[https://doi.org/10.1051/0004-6361/201218784|Detection of OD towards the Low-Mass Protostar IRAS 16293−2422]]**\\
 //Astron. Astrophys.// **542**, Art. No. L5 (2012).\\ //Astron. Astrophys.// **542**, Art. No. L5 (2012).\\
 +The GREAT receiver on board SOFIA was employed for the observations. A relatively high ratio of OD to HDO was found.\\ 
 +\\
  
 ---- ----
  • molecules/ism/oh.1785318049.txt.gz
  • Last modified: 2026/07/29 11:40
  • by mueller