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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 C4.

Same as Figure 3, but comparing effects of AM transport at different time moments between H. C. Spruit (2002)’s model (dashed lines) and J. Fuller et al. (2019)’s model (solid lines) used in main text. We assume ξTS = 1 and χTS = 1 in both cases.

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