A model analysis of the infrared data of late type stars surrounded by the circumstellar dust envelopes.

Details A model analysis of the infrared data of late type stars surrounded by the circumstellar dust envelopes. A model analysis of the infrared data of late type stars surrounded by the circumstellar dust envelopes.

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992srtoh..12..133h&link_type=abstract

Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 12, Nos. 2/3, p. 133 - 143

Physics

Scientific paper

A lot of model infrared spectral energy distributions of the oxygen-rich late type stars surrounded by the circumstellar dust envelopes are calculated by solving the radiative transport equations in the spherical dust envelope with various model input parameters. Using IRAS photometric data at 12, 25 and 60 μm and the strength of the silicate band feature at 10 μm from LRS spectra the best fit model is searched for each IRAS oxygen-rich evolved star with the circumstellar dust envelope.

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