Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaper › Journal article › Research › peer-review
Identification of stable configurations in the superhydrogenation sequence of polycyclic aromatic hydrocarbon molecules. / Jensen, Pernille A.; Leccese, Mirko; Simonsen, Frederik D.S. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 486, No. 4, 07.2019, p. 5492-5498.Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaper › Journal article › Research › peer-review
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TY - JOUR
T1 - Identification of stable configurations in the superhydrogenation sequence of polycyclic aromatic hydrocarbon molecules
AU - Jensen, Pernille A.
AU - Leccese, Mirko
AU - Simonsen, Frederik D.S.
AU - Skov, Anders W.
AU - Bonfanti, Matteo
AU - Thrower, John D.
AU - Martinazzo, Rocco
AU - Hornekær, Liv
PY - 2019/7
Y1 - 2019/7
N2 - Superhydrogenated polycyclic aromatic hydrocarbon (PAH) molecules have been demonstrated to act as catalysts for molecular hydrogen formation under interstellar conditions. Here we present combined thermal desorption mass spectrometry measurements and density functional theory calculations that reveal the most stable configurations in the superhydrogenation sequence of the PAH molecule coronene (C24H12). Specifically, the experiments demonstrate the presence of stable configurations of superhydrogenated coronene at specific hydrogenation levels of 2, 10, 14, 18, and 24 extra hydrogen atoms. Density functional theory calculations of binding energies and barrier heights explain why these configurations are particularly stable and provide new insights into the superhydrogenation process of PAH molecules under interstellar conditions. Furthermore, an experimental cross-section for the first hydrogen atom addition to the neutral coronene molecule of σadd = 2.7+2.7-0.9 × 10-2 A2 is derived from the experimental hydrogenation data.
AB - Superhydrogenated polycyclic aromatic hydrocarbon (PAH) molecules have been demonstrated to act as catalysts for molecular hydrogen formation under interstellar conditions. Here we present combined thermal desorption mass spectrometry measurements and density functional theory calculations that reveal the most stable configurations in the superhydrogenation sequence of the PAH molecule coronene (C24H12). Specifically, the experiments demonstrate the presence of stable configurations of superhydrogenated coronene at specific hydrogenation levels of 2, 10, 14, 18, and 24 extra hydrogen atoms. Density functional theory calculations of binding energies and barrier heights explain why these configurations are particularly stable and provide new insights into the superhydrogenation process of PAH molecules under interstellar conditions. Furthermore, an experimental cross-section for the first hydrogen atom addition to the neutral coronene molecule of σadd = 2.7+2.7-0.9 × 10-2 A2 is derived from the experimental hydrogenation data.
KW - ISM: clouds
KW - ISM: molecules
KW - Photodissociation region
U2 - 10.1093/mnras/stz1202
DO - 10.1093/mnras/stz1202
M3 - Journal article
AN - SCOPUS:85067919562
VL - 486
SP - 5492
EP - 5498
JO - Royal Astronomical Society. Monthly Notices
JF - Royal Astronomical Society. Monthly Notices
SN - 0035-8711
IS - 4
ER -