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Fig. 18
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Radial dependence of the molecular abundances normalized to their values at r=5 stellar radii (r*) of H 12CN (red), SiO and CO (black and blue) and CS (green) molecules, as predicted by a model of a C/O = 0.95 star hit by a shock of 25 km s−1 formed at one stellar radius (Cherchneff 2006).
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