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The hydrogen atoms of the fulleranes are expected to be located radially outward from the carbon atoms. 07 Å, see for example (Braga et al 1991). We assume the moment of inertia, IC, of a fullerene as that of a spherical cage with radius R: IC = 2/3NmcR², where mc is the mass of the carbon atom. 07 Å. The moment of inertia of the hydrogenated buckyonion will be taken as the sum of the moments of inertia of all the individual fullerenes conforming the molecule plus that of the layer of hydrogen atoms.

All the other elements can be considered as impurities. Hydrogen is present in the Universe both under atomic and under molecular form. Molecular hydrogen (H2) is the simplest and most abundant molecule in our cosmos but we have problems in explaining how molecular hydrogen can be formed for instance in the interstellar clouds. The problem of the formation Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Catania, Via S. es F. Cataldo and S. V. 2010 39 40 F. Cataldo and S. 48 eV per hydrogen molecule formed.

The abundances inferred for fullerenes are consistent with estimates for the carbon budget in the ISM. Hydrides of the fullerene C60 have also been investigated as potential DIB carriers (Webster 1992, 1993b). No specific identification has been suggested but it should be noted that the conjugated systems of p-electrons are predicted to have transitions in the visible range. The predicted optical and near-infrared transitions of fullerene based molecules may offer a potential explanation for the long-standing problem of the diffuse interstellar bands and other interstellar and circumstellar features.

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