Image Details
Caption: Figure 6.
Mass–radius diagram for transiting BDs (<80MJ). TOI-7019b (red star) occupies a unique position as a transiting BD orbiting the most metal-poor host known. Theoretical isochrones from the Sonora models (C. V. Morley et al. 2024) are shown for solar metallicity at ages of 0.1, 1, 4, and 10 Gyr.
© 2026. The Author(s). Published by the American Astronomical Society.