Figure 3 from A Family Picture: Tracing the Dynamical Path of the Structural Properties of Multiple Populations in Globular Clusters

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A Family Picture: Tracing the Dynamical Path of the Structural Properties of Multiple Populations in Globular Clusters

Authors: Emanuele Dalessandro, M. Cadelano, E. Vesperini, S. Martocchia, F. R. Ferraro, B. Lanzoni, N. Bastian, J. Hong, and N. Sanna

2019 The Astrophysical Journal Letters 884 L24.

Provider: AAS Journals

Caption: Figure 3.

Upper panel: distribution of ﹩{A}_{2}^{+}﹩ as a function of t/t_rh (N_h) for all the clusters in the sample. Bottom panel: zoom on the distribution of cluster with N_h < 30. Results from N-body models are overplotted to the observations. Blue and green curves represent models starting with an SP 5 and 10 times more centrally concentrated than FP, respectively.

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