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Mass-ratio Reversal as an Alternative to Hierarchical Mergers for GW241011

  • Authors: Rui-Chong Hu, Ying Qin, Bing Zhang

Rui-Chong Hu et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

Distribution of the effective spin parameter (χeff) as a function of the mass ratio (q) for MRR BBHs from the same model as in Figure 1. The population is partitioned by binary evolutionary channel: SMT (blue) and CE (orange). The blue contour denotes the 90% credible region inferred for GW241011.

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