Constraints on circumstellar dust grain sizes from high spatial resolution observations in the thermal infrared.

Details Constraints on circumstellar dust grain sizes from high spatial resolution observations in the thermal infrared. Constraints on circumstellar dust grain sizes from high spatial resolution observations in the thermal infrared.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339...81b&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 81 - 84

Physics

Circumstellar Dust: Infrared Surveys, Circumstellar Dust: Herbig Ae-Be Stars, Circumstellar Dust: Supergiants

Scientific paper

The authors describe how high spatial resolution imaging of
circumstellar dust at a wavelength of about 10 μm, combined with
knowledge of the source spectral energy distribution, can yield useful
information about the sizes of the individual dust grains responsible
for the infrared emission.

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