Modelling the evolution of pulsar wind nebulae

  • Michael Vorster

Abstract

Using numerical models, the influence of factors such as agnetic field strength on the evolution of pulsar wind ebulae can be determined. This includes the morphological evolution as well as the evolution of the type of light emitted and the corresponding intensity.
Published
2013-07-15
Section
Conference Abstract: Studentesimposium in die Natuurwetenskappe 2011