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Dynamical Formation of the GW190814 Merger

  • Authors: Manuel Arca Sedda

2021 The Astrophysical Journal Letters 908 L38.

  • Provider: AAS Journals

Caption: Figure 8.

Surface map showing the cluster velocity dispersion as a function of mass and half-mass radius. From left to right, black lines identify clusters with a velocity dispersion of 0.3, 2, 5, 10, 50, and 100 km s−1, respectively. The three black stars identify the typical values for Galactic YCs (Portegies Zwart et al. 2010), GCs (Harris 2010), and the Galactic NC (Feldmeier et al. 2014).

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