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Magnetic field evolution in magnetar crusts through three-dimensional simulations
Current models of magnetars require extremely strong magnetic fields to explain their observed quiescent and bursting emission, implying that the field strength within the star’s outer crust is orders of magnitude larger than the dipole component inferred from spin-down measurements. This presents a...
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| Publicado no: | Proc Natl Acad Sci U S A |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
National Academy of Sciences
2016
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4839425/ https://ncbi.nlm.nih.gov/pubmed/27035962 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1522363113 |
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