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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 1.

Schematization of the dynamical encounter driving the formation of an NS–BH binary in a dense stellar environment. We assume that either a roaming NS scatters over a BH-star (ST) binary (left panel, configuration BHSTNS) or vice versa (right panel, NSSTBH).

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