Supernovae Blast Waves in Proto-Dwarf Galaxies

作者: Alberto Noriego-Crespo , Peter Bodenheimer

DOI: 10.1017/S0252921100102945

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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.

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