Plasma Physics
Astrophysical jets are highly collimated streams of plasma that are ejected from the regions around compact astronomical objects, such as black holes or neutron stars. These jets can extend over vast distances and play a crucial role in the dynamics and evolution of the surrounding medium. Understanding astrophysical jets involves examining their formation mechanisms, which are closely related to magnetohydrodynamic (MHD) equations and approximations, as they describe the behavior of electrically conducting fluids in the presence of magnetic fields.
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