Magnetic fields in axisymmetric neutron stars
We derive general equations for axisymmetric Newtonian magnetohydrodynamics and use these as the basis of a code for calculating equilibrium configurations of rotating magnetized neutron stars in a stationary state. We investigate the field configurations that result from our formalism, which includ...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
2009-06.
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| Subjects: | |
| Online Access: | Get fulltext |
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