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Spinning Down Neutron-star Merger Remnants with the Tayler–Spruit Dynamo: Global Simulations Reveal the Formation of Massive Disks and Neutron-rich Ejecta

  • Authors: Harry Ho-Yin Ng, Elias R. Most

Harry Ho-Yin Ng and Elias R. Most 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 10.

Electron-fraction profiles at ﹩\bar{t}=385\,{\rm{ms}}﹩ for the ξTS = 0 (left) and ξTS = 1 (right) models. Cyan contours denote rest-mass density as defined in Figure 7.

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