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Stellar populations in the Magellanic Clouds: looking through the dust

Published online by Cambridge University Press:  01 December 2006

Guido De Marchi ,
Nino Panagia  and
Martino Romaniello
Guido De Marchi
Affiliation:
ESA, Space Science Department, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands email: gdemarchi@rssd.esa.int
Nino Panagia*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: panagia@stsci.edu
Martino Romaniello
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany email: mromanie@eso.org
*
†also INAF-HQ, Via del Parco Mellini 84, 00136 Rome, Italy; and Supernova Ltd., OYV #131, Northsound Road, Virgin Gorda, British Virgin Islands.
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Abstract

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We present the first results of our study of stellar populations in the Large and Small Magellanic Clouds based on multi-band WFPC2 observations of “random” fields taken as part of the “pure parallel” programme carried out with the HST as a service to the community.

Keywords

Hertzsprung-Russell diagramstars: fundamental parametersdustextinction
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 333 - 334
Copyright
Copyright © International Astronomical Union 2007

References

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