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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 1.

Three-dimensional volume rendering of the rest-mass density ρ at selected TA for cases in Table 1 along with the magnetic field lines. Green and white lines display magnetic field lines that are either confined in the stars (green) or extend from the stellar interior into the exterior (white). 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 approximately ∼76% opacity (gray).

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