Other
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.325.1487b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 325, Issue 4, pp. 1487-1496.
Other
16
Stars: Atmospheres, Circumstellar Matter, Stars: Variables: Other, Dust: Extinction, Infrared: Stars
Scientific paper
We explore the occurrence of dust in M-type Mira atmospheres and its effect on limb darkening under schematic assumptions about dust temperatures and dust particle properties. Dust particles that are thermodynamically coupled to the surrounding gas may form and may affect limb darkening, though only by very little in infrared continuum bandpasses. Dust particles that assume the equilibrium temperature given by the mean intensity of the radiation field only form under rare circumstances. Unexpectedly large or wavelength-dependent infrared continuum radii observed by interferometry are unlikely to be caused by atmospheric dust, except possibly near 1μm however, radius measurements may be significantly affected by molecular band contamination.
Bedding Tim R.
Jacob Andrew P.
Scholz Marek
Wood Peter R.
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