Abstract
Observations of 1–25 µm continuum emission and the interstellar infrared emission features in reflection nebulae are reviewed. These observations place important constraints on models of very small grains or large molecules such as PAHs, which these models must address in order to understand this fundamental component of interstellar dust.
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© 1989 IAU
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Sellgren, K. (1989). Infrared Emission from Reflection Nebulae. In: Allamandola, L.J., Tielens, A.G.G.M. (eds) Interstellar Dust. International Astronomical Union / Union Astronomique Internationale, vol 135. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2462-8_8
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DOI: https://doi.org/10.1007/978-94-009-2462-8_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-0449-4
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