Image Details
Caption: Figure 3.
Top panel: CMD of globular clusters observed with Gaia (Figure 3 in Gaia Collaboration et al. 2018). Colors from blue to red distinguish increasing metallicities. Bottom panel: theoretical RGB isochrones from PADOVA (A. Bressan et al. 2012) for t = 10 Gyr and [M/H] = −2.5 to 0.5. The isochrone for [M/H] = −0.57 (TRGB color at (F090W − F150W)0 = 1.65) is shown by the black line.
© 2026. The Author(s). Published by the American Astronomical Society.