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    In:  CASI
    Publication Date: 2016-06-07
    Description: There is an enormous range in the properties of stars that are losing mass. The red giants responsible for injecting roughly half or more of the material into the interstellar medium are reviewed. The physical properties are described for the out flowing gases. Broadband observation constaints on the dust are described by use of spectrum analysis. Circumstellar dust is identified by carbon-carbon and carbon-hydrogen bonds.
    Keywords: ASTROPHYSICS
    Type: NASA, Washington. Interrleationships among Circumstellar, Interstellar and Interplanetary Dust; p 3-18
    Format: application/pdf
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