Image Details
Caption: Figure 2.
The observed flat velocity Vf as it relates to the fitted V200 for pseudo-isothermal (left panel) and NFW (right panel) halos (P. Li et al. 2020). Filled points have formal uncertainties <20% in V200; open points are less accurate fits. The solid line shows Vf = V200. The gray line in the right panel shows Equation (2a) of H. Katz et al. (2019), which corresponds roughly to fv ≈ 1.4.
© 2026. The Author(s). Published by the American Astronomical Society.