Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 12.

One-dimensional plots at y = z = 0 at different times for models P1U2, P1U23, and P1U24. Left panel: density in log-scale. Gray dashed lines represent the NS initial radius RNS(t = 0). Right panel: magnetic field strength ∣Bmag∣, with the three lines superposed.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse