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On the Classification of Infrared Spectra from Circumstellar Dust ShellsWe present results from an ongoing effort to classify the infrared spectra produced by circumstellar dust shells. Earlier efforts concentrated on oxygen-rich dust shells from sources associated with the asymptotic giant branch (AGB). Here, we describe the expansion of our classification to include S stars, supergiants, and carbon stars.
Document ID
19970007835
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Sloan, G. C.
(NASA Ames Research Center Moffett Field, CA United States)
Little-Marenin, I. R.
(Wellesley Coll. MA United States)
Price, S. D.
(Phillips Lab. Hanscom AFB, MA United States)
Date Acquired
August 17, 2013
Publication Date
October 1, 1996
Publication Information
Publication: From Stardust to Planetesimals: Contributed Papers
Subject Category
Astronomy
Accession Number
97N14456
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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