molecules:ism:h3o-plus

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:h3o-plus [2026/02/05 12:56] muellermolecules:ism:h3o-plus [2026/02/05 13:04] (current) mueller
Line 50: Line 50:
  
 Hot, metastable hydronium was also observed toward Sgr B2(M) and toward W31C outside the Galactic center by\\ Hot, metastable hydronium was also observed toward Sgr B2(M) and toward W31C outside the Galactic center by\\
 +D. C. Lis, P. Schilke, E. A. Bergin, M. Gerin, J. H. Black, C. Comito, M. De Luca, B. Godard, R. Higgins, F. Le Petit, J. C. Pearson, E. W. Pellegrini, T. G. Phillips, and S. Yu\\ 
 +**[[https://doi.org/10.1088/0004-637X/785/2/135|Widespread Rotationally Hot Hydronium Ion in the Galactic Interstellar Medium]]**\\ 
 +//Astrophys. J.// **785**, (2014) Art. No. 135.\\ 
 +Values of //T//<sub>rot</sub> were (re) determined as 177 ± 54 K and 546 ± 80 K for Sgr B2(M), 172 ± 51 K and 424 ± 48 K for Sgr B2(N), and about 62 K and 360 K for W31C; fewer transitions were detected for this last source and only up to //J// = //K// = 9.\\ 
 +\\
  
 ---- ----
  • molecules/ism/h3o-plus.1770292608.txt.gz
  • Last modified: 2026/02/05 12:56
  • by mueller