Image Details
Caption: Figure 5.
(a): Prot–σvz relations for individual GBP − GRP bins using the method described in Section 3.2. (b): Ro–σvz relations, where Ro ≔ Protτc. Ro is converted from Prot in (a) using the convective turnover time, τc, calculated with a relation described in V. See et al. (2024). The red solid line shows the critical Rossby number where weakened magnetic braking is in effect (Rocrit = 1.866; J. L. van Saders et al. 2016; N. Saunders et al. 2024). The sections corresponding to the the features are shown on the figures.
© 2025. The Author(s). Published by the American Astronomical Society.