Abstract
It is shown that the 10–13 μ band observed in the spectra of some carbon stars could arise from simple hydrocarbon molecules, especially of the type C n H 2n . These molecules could be present in circumstellar dust shells which are responsible for the 1000 K black-body excess observed for these stars, and the emission band is produced by collisional excitation.
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Tarafdar, S.P., Wickramasinghe, N.C. Hydrocarbon molecules in carbon stars. Astrophys Space Sci 35, L41–L45 (1975). https://doi.org/10.1007/BF00637011
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DOI: https://doi.org/10.1007/BF00637011