Image Details
Caption: Figure 6.
Lyα escape fraction (﹩{f}_{{\rm{esc}}}^{{\rm{Ly}}\alpha }﹩) and offset to stellar counterparts (ΔdLyα) as functions of dust attenuation (AV) and Lyα line width (FWHM(Lyα)). In the lower left panel, we manually plot a dashed line indicating a limit trend of suppressing ΔdLyα as AV increasing.
© 2026. The Author(s). Published by the American Astronomical Society.