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Assembling GW231123 in Star Clusters through the Combination of Stellar Binary Evolution and Hierarchical Mergers

  • Authors: Lavinia Paiella, Cristiano Ugolini, Mario Spera, Marica Branchesi, Manuel Arca Sedda

Lavinia Paiella et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 3.

Masses and effective spin distributions for YCs, GCs, and NCs in our fiducial simulation. The metallicity is set to Z = 0.002. The contour lines refer to the 68%, 95%, 99% (solid line) and 99.99% (dotted–dashed line) contours. The 1D distributions are normalized to 1 and displayed in log scale.

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