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What is Pulsar Wind Nebula Dynamics about?

The document describes MHD simulations of a magnetized pulsar wind interacting with its surroundings. The simulations show that the pulsar wind nebula will be elongated due to the dynamical influence of toroidal magnetic fields, confirming previous analytical predictions. The simulations also show that the expansion of the pulsar wind nebula can be modeled with a standard power-law expansion rate, even though the magnetic fields dynamically influence the system. The results are applied to analyze the expans

Author

Okklos

Language

EN