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<p>A key step in gas-phase polycyclic aromatic hydrocarbon (PAH) formation involves the addition of acetylene (or other
alkyne) to σ-type aromatic radicals, with successive additions yielding more complex PAHs. A similar process can happen for N-
containing aromatics. In cold diffuse environments, such as the interstellar medium, rates of radical addition may be enhanced when
the σ-type radical is charged. This paper investigates the gas-phase ion-molecule … Show more
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