Abstract
Based on the even distribution of metals in Blue Compact Dwarfs (BCDs) spread all over their volume, we show that a large amount of stars (≥108 M⊙) are required to justify such a homogeneous metal abundance. We also show that such a mass would imply a large number of bursts similar to the ones presently energizing the giant nebulae. On the other hand, the underlying stellar population in BCDs can easily account for the mass required to justify the homogeneous metal abundance. We also review the recent results concerning the hydrodynamics of the matter reinserted by winds and supernovae in young, massive and compact superstar clusters. In particular we show that clusters undergoing the bimodal hydrodynamic solution, retain a large amount of the reinserted matter and this lowers their mechanical energy power as well as the amount of metals expected to mix with the ISM.
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Acknowledgements
My thanks to Elena Terlevich for a critical review of the manuscript. This study has been supported by CONACYT - México, research grant 60333 and the Spanish Ministry of Science and Innovation under the collaboration ESTALLIDOS (grant AYA2007-67965-C03-01) and Consolider-Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC.
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Tenorio-Tagle, G. (2012). On the Metallicity of Blue Compact Dwarfs. In: Papaderos, P., Recchi, S., Hensler, G. (eds) Dwarf Galaxies: Keys to Galaxy Formation and Evolution. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-22018-0_29
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DOI: https://doi.org/10.1007/978-3-642-22018-0_29
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