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Abstract: The notion of death line of rotating pulsars is applied to model ofoscillating neutron stars. It is shown that the magnetosphere of typicalnon-rotating oscillating stars may not contain secondary plasma to support thegeneration of radio emission in the region of open field lines of plasmamagnetosphere.



Author: B.J. Ahmedov, V.S. Morozova

Source: https://arxiv.org/







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