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Stellar Population Challenge: analysis of M67 with the VO

Published online by Cambridge University Press:  01 December 2006

M. Cerviño ,
R. Guitiérrez  and
E. Solano
M. Cerviño
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Camino Bajo de Huétor 50, 18008Spain email: mcs@iaa.es Spanish Virtual Observatory (SVO)http://svo.laeff.inta.es
R. Guitiérrez
Affiliation:
Laboratorio de Astrofísica Espacial y Física Fundamental (LAEFF-INTA), Apdo 50727, Madrid28080 email: raul@laeff.inta.es, esm@laeff.inta.es Spanish Virtual Observatory (SVO)http://svo.laeff.inta.es
E. Solano
Affiliation:
Laboratorio de Astrofísica Espacial y Física Fundamental (LAEFF-INTA), Apdo 50727, Madrid28080 email: raul@laeff.inta.es, esm@laeff.inta.es Spanish Virtual Observatory (SVO)http://svo.laeff.inta.es
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Abstract

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In this poster we present the analysis of the CMD of M67 (proposed in the Stellar Population Challenge) performed with VO applications. We found that, although the VO environment is still not ready to perform a complete analysis, its use provides highly useful additional information for the analysis. Thanks to the current VO framework, we are able to identify stars in the provided CMD that are not suitable for isochrone fitting. Additionally, we can complete our knowledge of this cluster extending the analysis to IR colors, which were not provided in the original data but that are available thanks to the VO. On the negative side, we find it difficult to access theoretical data from VO applications, so, currently, it is not possible to perform completely the analysis of the cluster inside the VO framework. However it is expected that the situation will improve in a near future.

Keywords

galaxies: star clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 173 - 174
Copyright
Copyright © International Astronomical Union 2007

References

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