Image Details
Caption: Figure 6.
Same as Figure 5 but for a different initial maximum grain size ﹩{a}_{\max }﹩ from 0.05 to 0.5 μm, assuming a fixed f high-J = 50% and η = 0.01. The disruption zone is more extended to the entire envelope as ﹩{a}_{\max }﹩ increases and ﹩{S}_{\max }﹩ decreases.
© 2022. The Author(s). Published by the American Astronomical Society.