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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 5.

Same as Figure 3, but showing all cases with different dynamo saturation parameters for an intermediate time ﹩\bar{t}=200\,{\rm{ms}}﹩. Black dashed line corresponds to the initial angular velocity.

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