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• W1526558110 abstract "We present recent results for the yields of Si and O, produced in the sputtering of SiO 2 by ions of different masses, and show the importance of sputtering by heavy particles at low streaming velocities. These data are incorporated in a C-shock model to study the erosion of interstellar grains and the release of silicon through non-thermal sputtering within the shock. Once in the gas phase, the atomic silicon reacts with O 2 and is rapidly transformed into SiO. The column densities of SiO thus calculated are compared with the observations of molecular outflows with a satisfactory agreement. In the postshock gas, SiO disappears from the gas phase through the reaction SiO(OH,H)SiO 2 and SiO 2 remains, unseen, in the cold dense gas. This could explain the extremely low upper limits of SiO deduced from observations of dark clouds." @default.
• W1526558110 created "2016-06-24" @default.
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• W1526558110 date "1997-01-01" @default.
• W1526558110 modified "2023-10-14" @default.
• W1526558110 title "Non thermal sputtering of grains and production of SiO in interstellar shocks" @default.
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• W1526558110 doi "https://doi.org/10.1017/s0074180900009281" @default.
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