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HCN and C2H2 in carbon stars
Published online by Cambridge University Press: 04 August 2017
Extract
At the low temperatures of cool carbon star atmospheres polyatomic molecules form. Most abundant of these for the temperature range 2500–3000 are HCN and C2H2 (Fig. 1).
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- I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
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- Copyright © Reidel 1984