Image Details
Caption: Figure 5.
Comparison of the rotational velocity distributions of open and globular clusters using the empirical CDFs of three open clusters of different ages (M67: red, NGC 188: blue, NGC 6791: green, and all: black) and the CDFs of high-density and low-density globular clusters (Figure 2 of F. R. Ferraro et al. (2023).
© 2026. The Author(s). Published by the American Astronomical Society.