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Chemical Abundances and Physical Parameters of H II Regions in the Magellanic Clouds

Published online by Cambridge University Press:  25 May 2016

R.E. Carlos Reyes
R.E. Carlos Reyes*
Affiliation:
Laboratório Nacional de Astrofísica, CNPq, Caixa Postal 21, CEP 37500-000, Itajubá, MG, Brazil Seminario Permanente de Astronomía y Ciencias Espaciales, FCF, UNM San Marcos, Lima, Perú

Abstract

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I present the results of the photoionization modeling of eleven H II regions in the Magellanic Clouds (MCs). A comparison of their abundances with other systems are also presented.

Type
Part 4. Detailed Chemical Abundances
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 282 - 284
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Carlos Reyes, R.E., et al. 1999a, in preparation Google Scholar
Carlos Reyes, R.E., et al. 1999b, in Science with Gemini Workshop , Florianópolis, SC, Brazil, in press Google Scholar
Hill, V., Barbuy, B., & Spite, M. 1997, A&A, 323, 461 and references therein Google Scholar
Esteban, C., et al. 1998, MNRAS, 295, 401 Google Scholar
Peimbert, M. 1993, RevMexAA, 27, 9 Google Scholar