Figure 5 from Dynamical Formation of the GW190814 Merger

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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 5.

Average number of BHs and NSs in binaries as a function of the cluster mass and for different times; from top to bottom the time considered is 12, 6, 3, 1, and 0.5 Gyr, respectively.

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