molecules:extragalactic:arh-plus_extragalactic

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
molecules:extragalactic:arh-plus_extragalactic [2022/04/04 12:45] muellermolecules:extragalactic:arh-plus_extragalactic [2022/04/04 12:53] (current) mueller
Line 13: Line 13:
 A. M. Jacob, K. M. Menten, F. Wyrowski, B. Winkel, D. A. Neufeld and B. S. Koribalski<br> A. M. Jacob, K. M. Menten, F. Wyrowski, B. Winkel, D. A. Neufeld and B. S. Koribalski<br>
 reported on\\ reported on\\
-**[[https://doi.org/10.1051/0004-6361/201527254|ArH<sup>+</sup> and H<sub>2</sub>O<sup>+</sup> Absorption towards Luminous Galaxies]]**\\+**[[https://doi.org/10.1051/0004-6361/202142544|ArH<sup>+</sup> and H<sub>2</sub>O<sup>+</sup> Absorption towards Luminous Galaxies]]**\\
 //Astron. Astrophys.// **659**, (2022) Art. No. 152.\\ //Astron. Astrophys.// **659**, (2022) Art. No. 152.\\
 +The //J// = 1 − 0 transition of <sup>36</sup>ArH<sup>+</sup> was detected with the APEX 12 m dish toward the nearby galaxies NGC 253, NGC 4945, and Arp 220. The molecular fraction of the gas traced by ArH<sup>+</sup> was estimated to be ~10<sup>−3</sup> and that it resides in gas volumes with low electon densities.\\ 
 +\\
  
 ---- ----
  • molecules/extragalactic/arh-plus_extragalactic.1649069157.txt.gz
  • Last modified: 2022/04/04 12:45
  • by mueller