Supernovae and the mass loss from primordial clouds.

Physics

Scientific paper

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Supernovae: Galaxy Formation, Supernovae: Mass Loss

Scientific paper

The influence of supernova explosions on the evolution of low mass primordial clouds is discussed. Because of the low escape velocity from a low mass cloud the radiative phase of SNR evolution has been taken into account. Making general assumptions about the star formation rate and the initial mass function, the SN explosion rate has been calculated. Numerical calculations on the variation of gas content with time show that if a low mass primordial cloud has a density as low as that of the present epoch dwarf E galaxies, the cloud will be destroyed by the SN explosion inside them.

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