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ISO Mid-Infrared Spectra of Reflection NebulaeOur goal is to test predictions of models attributing the IEFs to polycyclic aromatic hydrocarbons (PAHs). Interstellar models predict PAHs change from singly ionized to neutral as the UV intensity, Go, decreases.
Document ID
20060034575
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/18890
Authors
Werner, M.
Uchida, K.
Sellgren, K.
Houdashelt, M.
Date Acquired
August 23, 2013
Publication Date
December 1, 1999
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
reflection nebulae dust infrared astronomy

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