Chemical desorption of methanol induced by hydrogen abstraction–addition cycles on cold grain surfaces
Clicks: 3
ID: 323574
2026
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
0.0
/100
3 views
0 readers
AI Quality Assessment
Not analyzed
Readership in this journal
Ranked #167 of 900 articles by views in monthly notices of the royal astronomical society
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 900 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
Abstract We report ultra-high vacuum experiments on the non-thermal desorption of methanol (CH3OH) from cold dust-grain analogues under hydrogen-atom bombardment. Monolayer methanol films on polycrystalline gold, compact amorphous solid water (ASW, 10 ML) and 13CO ice (2 ML) are exposed to H atoms at 3.3 × 1012 cm−2 s−1 and Ts = 8–12 K for up to 40 min. Films are monitored in situ by reflection absorption infrared spectroscopy (RAIRS) and post-exposure by temperature-programmed desorption (TPD). The methanol content drops rapidly, plateauing after ~20 min. Because the elevated H2 background precludes gas-phase detection, the depletions are upper limits to the chemical desorption efficiency: 52 ± 8 per cent on gold (12 K) and 12 ± 3 per cent on ASW. Subtracting the maximum plausible contribution from undetected ice-phase products (≲ 15–20 per cent cumulatively) brackets the true efficiency to ~32–52 per cent on gold and ≲ 12 per cent on ASW. On 13CO, concurrent formation of 13CH3OH from CO hydrogenation prevents a quantitative measurement. We attribute the depletion to repeated H-abstraction and re-addition cycles on the methyl group. The process is most efficient on gold, where the physisorbed, closed-shell molecule couples only weakly to the metal’s phonon and electronic dissipation channels, and is suppressed on ASW, where the hydrogen-bonded network rapidly drains the reaction energy. Methyl-bearing interstellar complex organic molecules (iCOMs) are susceptible to analogous abstraction–addition loops, but are also efficiently formed on grain surfaces, so desorption selectivity cannot be separated from formation efficiency with the present data.
| Reference Key |
openalex_W7172396661
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | Kamel A. K. Gadallah, A Sow, E Congiu, S Baouche, F Dulieu |
| Journal | monthly notices of the royal astronomical society |
| Year | 2026 |
| DOI |
10.1093/mnras/stag1471
|
| URL | |
| Keywords | Keywords not found |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.