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Unidentified Infrared Emission Bands

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Encyclopedia of Astrobiology
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Definition

The term unidentified infrared emission (UIE) bands refers to a family of emission features observed in a variety of astronomical sources, including the aromatic features at 3.3, 6.2, 7.7, 8.6, and 11.3 μm; aliphatic features at 3.4 and 6.9 μm; and broad emission plateaus at 8, 12, and 17 μm, as well as a host of weaker features that are too broad to be atomic or molecular lines.

History

A family of strong infrared emission bands at 3.3, 6.2, 7.7, 8.6, 11.3, and 12.7 μm were first detected in the young carbon-rich planetary nebula NGC 7027 (Gillett et al. 1973; Russell et al. 1977) (Fig. 1) and in the reflection nebula HD 44179 (Russell et al. 1978). Since the initial discovery, these features are now widely observed in HII regions, reflection nebulae, planetary nebulae, protoplanetary nebulae, and the diffuse interstellar medium of our own and other galaxies.

Fig. 1
figure 1

Infrared Space Observatory (ISO) spectrum of the planetary nebula NGC 7027 showing the UIE bands (labeled in red...

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References and Further Reading

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Kwok, S. (2014). Unidentified Infrared Emission Bands. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5077-4

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