The magnetic configuration in the plasma-sphere surrounding a neutron star is described in terms of a model equation that is constructed to be valid from the surface of the star to distances of the order of the light speed cylinder and beyond. Significant asymptotic solutions of this equation, that
An equatorially symmetric rotator model for magnetic stars
โ Scribed by L. Oetken
- Publisher
- John Wiley and Sons
- Year
- 1977
- Tongue
- English
- Weight
- 728 KB
- Volume
- 298
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
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