Energetic parameters used in the different astrochemical modeling simulations: energy barriers of the forward (Ea,for) and reverse (Ea,rev) reactions, and transition frequency of the transition state (ν≠).
|System||Reaction||Ea,for (K)||Ea,rev (K)||ν≠ (cm-1)||Reference|
|W32||CO + H → HCO||1106||11 290||569.7||this work|
|H2CO + H → CH3O||1299||15 880||701.3||this work|
|Gas-phase||CO + H → HCO||1979||8909||793.6||Peters et al. (2013)|
|H2CO + H → CH3O||2396||27 290||1037.0||Peters (2013)|
|laboratory ices||CO + H → HCO||390–520||Fuchs et al. (2009)|
|H2CO + H → CH3O||415–490||Fuchs et al. (2009)|
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.