Figure 5 from Modeling Dense Star Clusters in the Milky Way and beyond with the Cluster Monte Carlo Code

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Modeling Dense Star Clusters in the Milky Way and beyond with the Cluster Monte Carlo Code

Authors: Carl L. Rodriguez, Newlin C. Weatherford, Scott C. Coughlin, Pau Amaro-Seoane, Katelyn Breivik, Sourav Chatterjee, Giacomo Fragione, Fulya Kıroğlu, Kyle Kremer, Nicholas Z. Rui, Claire S. Ye, Michael Zevin, and Frederic A. Rasio

2022 The Astrophysical Journal Supplement Series 258 22.

Provider: AAS Journals

Caption: Figure 5.

An example snapshot of a realistic cluster model after 12 Gyr of evolution. On the left, we show a synthetic HST observation of the cluster, computing using the stellar positions, effective temperatures, and radii (via the Fresco package; Rieder & Pelupessy 2019). On the right, we show the V-band surface brightness profile (at a distance of 5 kpc) and 1D velocity dispersion for the cluster, calculated using the cmctoolkit package (Rui et al. 2021a).

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