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- W2039186954 startingPage "137" @default.
- W2039186954 abstract "Superluminal motion is often observed in extragalactic jets, but few simulations take into account the nature of relativistic fluids. Here, I have studied the behaviour of steady-state, supersonic jets propagating with a relativistic bulk velocity through a pressure gradient, similar to the observed atmospheres of extragalactic radio source hosts. The simulations were carried out in axisymmetry, using a Godunov-type fluid code in Lagrangian coordinates. The equation of state for a two-component ‘Synge gas’ was employed to close the system of conservation equations." @default.
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- W2039186954 date "1994-07-01" @default.
- W2039186954 modified "2023-09-25" @default.
- W2039186954 title "Simulation of relativistic jets" @default.
- W2039186954 doi "https://doi.org/10.1093/mnras/269.1.137" @default.
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