Galactic winds (or "outflows") are made up of gas driven out of galaxies by energy released from star formation related activity (supernovae), or by accretion of matter onto a supermassive black hole. During a starburst-driven wind, supernova bubbles within the galactic disk overlap and begin to collectively drive motion which propagates from scales of just a few parsecs, out to tens of kiloparsecs away. This volume rendering highlights the density structure of an idealized galactic wind simulation.
Methods: CHOLLA code; NVIDIA IndeX renderer