
%0 Journal Article
%A Burman, RR 
%T Sub-rotation and Super-rotation in Pulsar Magnetospheres
%J Australian Journal of Physics
%D 1981/02/01
%V 34
%N 1
%P 97-104
%K 
%R https://doi.org/10.1071/PH810097
%U https://www.publish.csiro.au/paper/PH810097 
%X 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. 
