HAL (France)
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Photodissociation of [Fe<sub>x</sub>(C<sub>24</sub>H<sub>12</sub>)<sub>y</sub>]<sup>+</sup> complexes in the PIRENEA setup: iron-polycyclic aromatic hydrocarbon clusters as candidates for very small interstellar grains.
Astronomical observations suggest that polycyclic aromatic hydrocarbons (PAHs) that emit at the surface of molecular clouds in the interstellar medium are locally produced by photodestruction of very small grains (VSGs). In this paper, we investigate [Fex(PAH)y]+ clusters as ca
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