Sub-rotation and Super-rotation in Pulsar Magnetospheres
For magnetospheric species that are nonrelativistic at the stellar surface in the general oblique rotator model, it is shown that a ondissipative flow branch which is sub-rotating when near the star remains sub-rotating everywhere, but that one which is super-rotating when near the star can become sub-rotating inside the light cylinder. Hence, both flow branches can cross the light cylinder and remain valid outside it.
1988 ◽
Vol 132
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pp. 329-332
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1986 ◽
Vol 90
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pp. 141-147
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1976 ◽
Vol 32
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pp. 577-588
1977 ◽
Vol 178
(2)
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pp. 61-70
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1974 ◽
Vol 166
(1)
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pp. 113-121
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1970 ◽
Vol 4
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pp. 269-273
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1985 ◽
Vol 6
(2)
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pp. 127-129
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