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Chemical abundances of the LMC cluster Hodge 11 and its surrounding field

Published online by Cambridge University Press:  18 January 2010

Renee Mateluna ,
Douglas Geisler  and
Sandro Villanova
Renee Mateluna
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Esteban Iturra s/n Barrio Universitario, Concepción, Chile email: renee@astro-udec.cl
Douglas Geisler
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Esteban Iturra s/n Barrio Universitario, Concepción, Chile email: renee@astro-udec.cl
Sandro Villanova
Affiliation:
Departamento de Astronomía, Universidad de Concepción, Esteban Iturra s/n Barrio Universitario, Concepción, Chile email: renee@astro-udec.cl
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Abstract

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We have obtained high-resolution VLT/FLAMES spectra of a number of giants in the LMC cluster Hodge 11 and the surrounding field. We present results of a detailed model-atmosphere abundance analysis for a variety of elements, including Fe, Ca, Ti, Si, Sc, Ni and Cr.

Keywords

galaxies: abundancesgalaxies: star clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 474 - 476
Copyright
Copyright © International Astronomical Union 2010

References

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