Image Details
Caption: Figure 4.
Distribution of ﹩{A}_{2}^{+}﹩ as a function of the ratio between the present-day and the initial cluster mass (﹩{M}_{\mathrm{PD}}/{M}_{\mathrm{ini}}﹩) obtained by Baumgardt et al. (2019). Blue and green curves represent the same models shown in Figure 3.
© 2019. The American Astronomical Society. All rights reserved.