The Physics of Rotating Magnetic Neutron Stars
- 1 March 1969
- journal article
- other
- Published by Cambridge University Press (CUP) in Publications of the Astronomical Society of Australia
- Vol. 1 (5) , 227-228
- https://doi.org/10.1017/s1323358000011668
Abstract
Gold has suggested that pulsars are rotating neutron stars with strong magnetic fields. We have studied the simplest such model, one having an external dipole field aligned with the rotation axis.Keywords
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