Dehydrogenation of polycyclic aromatic hydrocarbons in the diffuse interstellar medium

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dc.creatorVuong, My Ha
dc.creatorFoing, Bernard H.
dc.date2000-10-19
dc.date.accessioned2026-07-07T01:56:06Z
dc.date.available2026-07-07T01:56:06Z
dc.descriptionWe present a model for the hydrogenation states of Polycyclic Aromatic Hydrocarbons (PAHs) in the diffuse interstellar medium. First, we study the abundance of hydrogenation and charge states of PAHs due to photo-ionization, photo-dissociation in the interstellar UV field, electron recombination and chemical reactions between PAH cations and H or H_2. For PAH cations, we find that the dehydrogenation effects are dominant. The hydrogenation state of PAHs depends strongly on the H density, the size of the molecule and UV field. In diffuse clouds with low H density and normal UV radiation, PAHs containing less than 40 C are completely or strongly dehydrogenated whereas at high H density, they are normally hydrogenated. The partially dehydrogenated species dominate in intermediate density clouds. PAHs above 40 C are quite stable and are fully hydrogenated, which would favor their spectroscopic search in near IR surveys of Diffuse Interstellar Bands (DIBs).
dc.description4 Pages, including 5 PostScript figures. Accepted for publication in the Astronomy & Astrophysics letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0010385
dc.identifierhttp://arxiv.org/abs/astro-ph/0010385
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1880
dc.subjectAstrophysics
dc.titleDehydrogenation of polycyclic aromatic hydrocarbons in the diffuse interstellar medium
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