Physics
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.489o&link_type=abstract
IAU Symposium No. 135: Interstellar dust: contributed papers, p. 489 - 494
Physics
M Stars: Circumstellar Dust, Formation: Circumstellar Dust
Scientific paper
The author calculates model spectra taking account of silicate mantle
growth and investigates the physical parameters which may determine the
appearance of the 9.7 μm feature in M Mira variables.
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