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Simulations, Data Analysis and Algorithms

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Figure 4 | Computational Astrophysics and Cosmology

Figure 4

From: Stationary relativistic jets

Figure 4

Accuracy of the ultra-relativistic hot jets solution for the model with atmospheres with \(\pmb{\kappa=2}\) . The left panel shows the Lorentz factor at \(z=9\) for models with 150 (dotted), 300 (dot-dashed), 600 (dashed line) and 1,200 (solid line) grid points. The right panel show the total energy flux as a function of the distance from the nozzle for the model with 300 grid points.

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