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Hydrated sulphuric acid in dense molecular clouds
Authors:Flavio Scappini  Cesare Cecchi-Pestellini  Harvey Smith  William Klemperer  Alexander Dalgarno
Institution:Istituto per lo Studio dei Materiali Nanostrutturati del CNR, Via P. Gobetti 101, 40129 Bologna, Italy;Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA;Department of Chemistry, Harvard University, 12 Oxford Street, Cambridge, MA 02138, USA
Abstract:We consider sulphur depletion in dense molecular clouds, and suggest hydrated sulphuric acid, H2SO4 ·  n H2O, as a component of interstellar dust in icy mantles. We discuss the formation of hydrated sulphuric acid in collapsing clouds and its instability in heated regions in terms of the existing hot core models and observations. We also show that some features of the infrared spectrum of hydrated sulphuric acid have correspondence in the observed spectra of young stellar objects.
Keywords:ISM: clouds  dust  extinction  ISM: lines and bands  ISM: molecules  infrared: ISM
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