Image Details
Caption: Figure 17.
Same as Figure 16 but for various values of f high-J from 25% to 100%, assuming a fixed ﹩{S}_{\max }={10}^{9}\,\mathrm{erg}\,{\mathrm{cm}}^{-3}﹩ and η = 0.002.
© 2022. The Author(s). Published by the American Astronomical Society.