On the evolution of supernova remnants. II - Two-dimensional calculations of explosions inside pre-existing wind-driven bubbles
Supernova explosions within wind-driven bubbles are studied with 2D hydrodynamical calculations. Two different density distributions for the ejecta are considered: (1) a smooth, unfragmented power-law stratification, and (2) a fragmented distribution. As in 1D models, the presence of the shell of interstellar swept-up matter causes the rapid
Tenorio-Tagle, G. et al.
Fecha de publicación:
7
1991