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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 1.

Resistivity profiles along the radial direction for our fiducial simulation with B p = B 6.5. The two lines refer to the choice of a wide resistive transition layer (red dashed line) and corresponding to the one adopted in Ciolfi et al. (2011), or of a thin layer (blue solid line). The vertical line marks the radius of the star R.

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