作者: Alberto Noriego-Crespo , Peter Bodenheimer
DOI: 10.1017/S0252921100102945
关键词:
摘要: Gas mass loss in proto-dwarf galaxies can be efficiently driven out by blast waves created by the first generation of supernovae. There is, however, a threshold set by the total gravitational potential beyond which gas mass loss does not occur. This limit is in agreement with the one predicted by some Cold Dark Matter senarios.