Variations of P2 in subpulse drifting pulsars
We develop a model for subpulse separation period, P2, taking into account both the apparent motion of the visible point as a function of pulsar phase, ψ, and the possibility of abrupt jumps between different rotation states in non-corotating pulsar magnetospheres. We identify three frequencies: (i)...
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| Main Authors: | , , , , |
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| Format: | Article |
| Published: |
Oxford University Press
2016
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| Subjects: | |
| Online Access: | http://eprints.um.edu.my/18750/ http://dx.doi.org/10.1093/mnras/stw679 |
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