Physics
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..379b&link_type=abstract
Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe
Physics
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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