Abstract
The interstellar medium (ISM) is a complex physical and chemical environment which gives rise to a variety of spectral features. This chapter gives a brief overview on the diversity of chemical species that are observed in diffuse interstellar clouds, tenuous entities of gas, and dust scattered throughout the galaxy and beyond. The growing evidence for the existence of large organic, prebiotic molecules in these astrophysical environments is discussed.
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Cox, N. (2012). Molecules Between the Stars. In: Hanslmeier, A., Kempe, S., Seckbach, J. (eds) Life on Earth and other Planetary Bodies. Cellular Origin, Life in Extreme Habitats and Astrobiology, vol 24. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-4966-5_6
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