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PLANETARY NEBULAE AND THE CHEMICAL EVOLUTION OF THE MAGELLANIC CLOUDS

The determination of accurate chemical abundances of planetary nebulae (PN) in di erent galaxies allows us to obtain important constraints on chemical evolution models for these systems. We have a long-term program to derive abundances in the galaxies of the Local Group, particularly the Large and S...

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Bibliografske podrobnosti
izdano v:Revista Mexicana de Astronomía y Astrofísica
Main Authors: W. J. Maciel, R. D. D. Costa, T. E. P. Idiart
Format: Artigo
Jezik:Inglês
Izdano: Universidad Nacional Autónoma de México 2009
Teme:
Online dostop:https://www.redalyc.org/articulo.oa?id=57112175001
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