Image Details
Caption: Figure 11.
Same as Figure 10 but for a fixed ﹩{S}_{\max }={10}^{9}\,\mathrm{erg}\,{\mathrm{cm}}^{-3}﹩ and varied f high-J , ranging from 25% to 100%. The total-to-selective ratio R V tends to rise with a lower fraction of grains at high-J attractors in the CSE.
© 2022. The Author(s). Published by the American Astronomical Society.