Fig. B.1

Particle size as a function of distance to the star. The red, green, and blue lines represent for αacc = 10−2, 10−3, and 10−4, respectively (Eq. (B.3)). The Stokes regime is where
, while the Epstein regime is where
. Four black and gray lines represent particle size whose τs = 0.3, 0.1, 0.03, and 0.01 in the Stokesregime and the Epstein regime with αacc = 10−2, respectively. Here, Ṁg = 10−8M⊙ yr−1 and
are used.
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