Image Details
Caption: Figure 8.
Same as Figure 7 but with f high-J ranging from 25% to 100%, assuming compact grains with ﹩{S}_{\max }={10}^{9}\,\mathrm{erg}\,{\mathrm{cm}}^{-3}﹩. The enhancement of grains at high-J attractors being disrupted by RATs causes increased far-UV extinction and decreased optical–IR extinction.
© 2022. The Author(s). Published by the American Astronomical Society.