Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

The Swept-back Multipolar Magnetic Field of Neutron Stars: Application to NICER MSP J0030+0451

  • Authors: Anu Kundu, Constantinos Kalapotharakos, Zorawar Wadiasingh, Greg Olmschenk, Wendy F. Wallace, Alice K. Harding, Christo Venter, Demosthenes Kazanas

Anu Kundu et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

The x- and y-axes indicate the indices l and m, respectively, while the colors represent the absolute magnitude of the multipolar coefficients, ﹩| {a}_{lm}^{B,{\rm{in}}}| ﹩, on the stellar surface. The log-linear color bar shows the true values. Each panel corresponds to one of the vacuum solutions of CK21. All m = {0, …, l} cases are shown up to l = 20.

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