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Infrared Emission from Reflection Nebulae

Published online by Cambridge University Press:  23 September 2016

K. Sellgren
K. Sellgren*
Affiliation:
Institute for Astronomy, University of Hawaii

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 135: Interstellar Dust , 1989 , pp. 103 - 108
Copyright
Copyright © Kluwer 1989 

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