
TY  - JOUR
A1  - Burman, RR 
T1  - Sub-rotation and Super-rotation in Pulsar Magnetospheres
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1981
VL  - 34
IS  - 1
SP  - 97
EP  - 104
KW  - 
UR  - https://doi.org/10.1071/PH810097 
N2  - 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. 
ER  -

