franco_vazza<p>Latest formation stages (approximately from redshift z=1 to z=0) of a massive cluster of galaxies which undergoes mergers along the diagonal direction of the image.<br>The left panel shows the evolving baryon density, the central one the temperature (which marks shocks driven by mergers) and the right one the magnetic field intensity.</p><p>ENZO simulations at CINECA (Italy) with <a href="https://mastodon.social/tags/Julialang" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Julialang</span></a> post-processing.</p><p><a href="https://mastodon.social/tags/SimulatedUniverses" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>SimulatedUniverses</span></a> <a href="https://mastodon.social/tags/astronomy" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>astronomy</span></a> <a href="https://mastodon.social/tags/science" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>science</span></a> <a href="https://mastodon.social/tags/physics" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>physics</span></a></p>