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

Authors: Yi-Xian Chen, Brian D. Metzger

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

Provider: AAS Journals

Caption: Figure 3.

For the fiducial slow cooling (nonfragmenting) simulation, a typical snapshot showing the (x, y) profiles through the midplane (z = 0) of density, temperature, local cooling time, equilibrium electron fraction, and chemical potential. Lengths are expressed in units of the vertical scale height H.

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