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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 10.

Strength of the magnetic field for P1U4 at selected times. White lines indicate the field lines. Notice that the color-bar limits are rescaled, using ﹩{B}_{{\rm{\max }}}﹩ at each time to account for changes in field strength. Similar behavior is observed across the other rotating cases.

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