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Impact of Rotation on Magnetic Field Stability and Orientation in Isolated Neutron Stars

  • Authors: Fabrizio Venturi Piñas, Anson Ka Long Yip, Patrick Chi-Kit Cheong, Milton Ruiz

Fabrizio Venturi Piñas et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

Top view of the rest-mass density of P1U4, along with the field lines at TA = 0 (left panel) and near to the end of the simulation (≈12.5TA). The color bar (logarithmic scale) ranges from the atmospheric density to the maximum rest-mass density at the corresponding time. The black and gray rectangles to the left of the color bar indicate opacity, which ranges from fully opaque (black) to ∼76% opacity (gray).

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