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Infrared Emission from Reflection Nebulae
Published online by Cambridge University Press: 23 September 2016
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.
- Type
- Section II: The Overidentified Infrared Emission Features
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- Copyright © Kluwer 1989