期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 479, 期 1, 页码 649-656出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/sty1528
关键词
astrochemistry; molecular processes; ISM: molecules
We present experimental data on H-2 formation processes on gas-phase polycyclic aromatic hydrocarbon (PAM cations. This process was studied by exposing coronene radical cations, confined in a radio-frequency ion trap, to gas-phase H atoms. Sequential attachment of up to 23 hydrogen atoms has been observed. Exposure to atomic D instead of H allows one to distinguish attachment from competing abstraction reactions, as the latter now leave a unique fingerprint in the measured mass spectra. Modelling of the experimental results using realistic cross-sections and barriers for attachment and abstraction yield a 1:2 ratio of abstraction to attachment cross-sections. The strong contribution of abstraction indicates that H-2 formation on interstellar PAH cations is an order of magnitude more relevant than previously thought.
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