Release of large polycyclic aromatic hydrocarbons and fullerenes by cosmic rays from interstellar dust Swift heavy ion irradiations of interstellar carbonaceous dust analogue : Release of large polycyclic aromatic hydrocarbons and fullerenes by cosmic rays from interstellar dust Swift heavy ion irradiations of interstellar carbonaceous dust analogue
Context. Top-down chemistry is believed to be responsible for the formation of the large molecular compounds such as the polycyclicaromatic hydrocarbon-like molecules and the fullerenes observed in the interstellar medium. The release of these large molecules fromthe parent grains remains an important issue to be investigated.Aims. Cosmic rays irradiate the dust grains during their journey in the
