Observational constraints on interstellar dust models.

Details Observational constraints on interstellar dust models. Observational constraints on interstellar dust models.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.391h&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 391 - 393

Computer Science

Interstellar Grains: Models, Interstellar Grains: Infrared Radiation, Interstellar Grains: Uv Radiation

Scientific paper

No single model has been able to account for all of the observed spectroscopic properties of interstellar or circumstellar dust. The reason for this is that there is strong disagreement as to their exact structure and composition. The authors examine recent UV and IR data and attempt to put constraints on the possible types of interstellar grain composition, and to connect these constraints with grain models.

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