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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 11.

Total surface magnetic field for the best-fit solutions, with DQ on top and DQO at the bottom, on a Mollweide projection. The color bar represents normalized value, with 1 being the maximum value on the surface, which is given on top of every subplot as ﹩{B}_{{\rm{\max }}}﹩ (in terms of the dipolar field BD = 1). The contours of the corresponding hotspots are overlaid on top in white.

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