Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-06-23
Astronomy and Astrophysics
Astrophysics
8 pages, 3 figures, 2 table, Accepted for publication in ApJ
Scientific paper
10.1086/322960
We construct three extreme different scenarios of the star formation histories applicable to a sample of dwarf galaxies, based either on their present metallicity or their luminosity. The three possible scenarios imply different mechanical energy input rates and these we compare with the theoretical lower limits established for the ejection of processed matter out of dwarf galaxies. The comparison strongly points at the existence of extended gaseous haloes in these galaxies, acting as the barrier that allows galaxies to retain their metals and enhance their abundance. At the same time our findings strongly point at a continuous star-forming process, rather than to coeval bursts, as the main contributors to the overall metallicity in our galaxy sample.
Cervino Miguel
Kunth Daniel
Legrand François
Silich Sergiy
Tenorio-Tagle Guillermo
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