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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 8.

Ratio of specific angular momentum to the ISCO value as a function of mass coordinate. The ISCO quantity is computed self-consistently from the enclosed mass and its total angular momentum at each mass coordinate. Each curve corresponds to one stellar model. The vertical black line marks the location of the 3 M⊙ mass coordinate.

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