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The Composition of Interstellar Grains and IcesImmense progress has been made in our understanding of the composition of interstellar dust over the past 15 years. This progress is largely due to the synergism of improved telescopic observations (especially in the infrared), laboratory studies of dust analogs, and the study of the interstellar grains found in meteorites. This paper reviews our current understanding of the composition of interstellar dust in light of results obtained by these three disciplines.
Document ID
20020034921
Acquisition Source
Ames Research Center
Document Type
Abstract
Authors
Sandford, Scott A. (NASA Ames Research Center Moffett Field, CA United States)
Witteborn, Fred C.
Date Acquired
August 20, 2013
Publication Date
January 1, 1995
Subject Category
Astrophysics
Funding Number(s)
PROJECT: RTOP 452-22-94-06
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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