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Organic Molecules in Interstellar Dust: A Possible Spectral Signature at λ2200 Å?

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Abstract

The λ2 200 Å interstellar absorption band, generally attributed to graphite grains, could equally well arise from π→* electronic transitions in conjugated double bonds of organic molecules. These molecules, which should comprise ∼ 10% of the total interstellar dust mass, may be lodged within clumps of 100 Å-sized refractory grains.

1977, Astrophys. Space Sci. 47, L9-L11

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Wickramasinghe, N.C., Hoyle, F., Nandy, K. (2000). Organic Molecules in Interstellar Dust: A Possible Spectral Signature at λ2200 Å?. In: Hoyle, F., Wickramasinghe, N.C. (eds) Astronomical Origins of Life. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4297-7_30

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  • DOI: https://doi.org/10.1007/978-94-011-4297-7_30

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