Image Details
Caption: Figure 9.
As Figure 8, but with galaxies color coded according to their membership class (as listed in Table 5). Certain (Membership Class 0), likely (Membership Class 1), and possible (Membership Class 2) members are shown separately in the three smaller panels to the right. The fourth small panel on the bottom right shows the 10 galaxies classified as Virgo members based on our photometric/structural criteria, but subsequently shown to have velocities above 3500 km s−2.
© 2026. The Author(s). Published by the American Astronomical Society.