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Simulations, Data Analysis and Algorithms

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Figure 1 | Computational Astrophysics and Cosmology

Figure 1

From: Stationary relativistic jets

Figure 1

Reconfinement of the \(\pmb{M_{\mathrm{j}}=15}\) , \(\pmb{T_{\mathrm{j}}=\sqrt{10}\times10^{13}\mathrm{K}}\) jet. The top panel is a reproduction of Figure 3 from B94. The bottom panel shows the solution obtained with our method. In each panel, the top halves show 50 pressure contours (spaced by the factor of 1.18) and the bottom halves show the temperature parameter \(\tau\equiv\rho h/(\rho h - p)\) in 50 contours (spaced by the factor of 1.003). The light gray lines are streamlines.

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