Stellar feedback in dwarf galaxies: the case of IC 5152

Physics

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Scientific paper

We analyze the massive stellar content and its feedback onto the interstellar medium of the very isolated dwarf galaxy IC 5152. Deep Hα imaging show a pervasive diffuse ionized medium with shell and filament structures from small to large scales. The current star formation rate is high. Preliminary analysis of a HST based color-magnitude diagram support a strong current starformation activity and significant star formation at least 1 Gyr ago.

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