Observational constraints on circumstellar dust

Details Observational constraints on circumstellar dust Observational constraints on circumstellar dust

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2403....3j&link_type=abstract

Interrelationships among Circumstellar, Interstellar, and Interplanetary Dust, Proceedings of the Workshop held 27 February - 1

Physics

8

Cosmic Dust, Radiation Pressure, Red Giant Stars, Stellar Envelopes, Stellar Mass Ejection, Carbon Monoxide, Flow Velocity, Grain Size, Hydrogen, Infrared Spectra, Radio Spectra

Scientific paper

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.

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