Image Details
Caption: Figure 6.
Left panel: Roche filling factor as a function of NUV flux at the planet’s orbit for survey targets and planets orbiting early-type stars with published mass-loss measurements. Right panel: retrieved mass-loss rates as a function of NUV flux at the planet’s orbit. See the Figure 5 caption for additional details.
© 2026. The Author(s). Published by the American Astronomical Society.