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Dust grain radius
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Radius of silicate grains: 0 .. 1 μm (
mp4
)
model st28gm06n074, α
stick
=0.1
Stellar interior and (very) inner atmosphere:
too hot to form dust
Outer atmosphere:
dust forms in dense non-sperical blobs
dust clouds might be shortlived
or stable causing a stellar wind, driven by radiation pressure on dust grains