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Multi-wavelength emission modelling of PSR J0437–4715

Context. The diversity of pulsar light curves and radio polarisation properties originates in the structure of the magnetic field close to the stellar surface. For millisecond pulsars, this complexity is particularly puzzling. Fortunately, some means exist to uncover the magnetic field topology that...

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Principais autores: Pétri J., Stammler P., Guillemot L., Guillot S., González-Caniulef D., Jankowski F., Webb N.
Format: Artigo
Sprog:Inglês
Udgivet: EDP Sciences 2026-04-01
Serier:Astronomy & Astrophysics
Fag:
magnetic fields
methods: numerical
pulsars: general
stars: rotation
pulsars: individual: psr j0437–4715
Online adgang:https://www.aanda.org/articles/aa/full_html/2026/04/aa58077-25/aa58077-25.html
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