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Gravitational Instability and Fragmentation in Collapsar Disks Supports the Formation of Subsolar Neutron Stars

Yi-Xian Chen and Brian D. Metzger 2025 The Astrophysical Journal Letters 991 .

Caption: Figure 9.

Same as Figure 6 but illustrating the bound clump properties for model O8T1e10, corresponding to an initially α-rich disk.