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Poloidal-field Instability in Magnetized Relativistic Stars

  • Authors: Riccardo Ciolfi and Luciano Rezzolla

Ciolfi & Rezzolla 2012 The Astrophysical Journal 760 1.

  • Provider: AAS Journals

Caption: Figure 5.

Instability growth time as a function of the initial magnetic-field strength (black circles). The red dashed line represents a fitted linear scaling as expected from perturbation theory.

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