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Jets from Scratch: Dynamo-generated Poloidal Magnetic Fields in Three-dimensional Collapsar Simulations

  • Authors: Ho-Sang Chan, Ore Gottlieb, Jonatan Jacquemin-Ide, Matteo Cantiello, Mathieu Renzo

Ho-Sang Chan et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 9.

Panel (a): time-averaged (solid blue line) profile of the collapsar-disk scale height measured with respect to the midplane, where the shaded region denotes one standard deviation from the mean. Panel (b): same as panel (a), but for the mass-weighted angular-velocity profile. The black dashed line shows the Keplerian angular velocity, Ωkep = 1/(r3/2 + a). In both panels, the text box indicates the model. The time averaging is performed before the first jet is launched.

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