Supergalactic Winds Driven by Multiple Super-Star Clusters
Here we present two-dimensional hydrodynamic calculations of free expanding supergalactic winds, taking into consideration strong radiative cooling. Our main premise is that supergalactic winds are powered by collections of super-star clusters, each of which is a source of a high-metallicity supersonic diverging outflow. The interaction of winds
Tenorio-Tagle, Guillermo et al.
Fecha de publicación:
11
2003