Skip to main content

Simulations, Data Analysis and Algorithms

Computational Astrophysics and Cosmology Cover Image
Figure 2 | Computational Astrophysics and Cosmology

Figure 2

From: Stationary relativistic jets

Figure 2

Ultra-relativistically hot jets (Kohler et al. 2012 ; Kohler and Begelman 2015 ) in power-law atmospheres with \(\pmb{\kappa=8/3,7/3}\) and 2 (from left to right). The color-coded images show the distribution of the Lorentz factor. The initial Lorentz factor is \(\Gamma_{0}=50\) and opening angle \(\theta_{0}=1/\Gamma_{0}\).

Back to article page
\