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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 8.

Mass-ejection rate, ﹩{\dot{M}}_{{\rm{ej}}}﹩, computed at a spherical radius of 550 km for all simulated dynamo saturation parameters, ξ_TS.

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