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The Spitzer Survey of the Large Magellanic Cloud: SAGE, A Review of Initial Results

Published online by Cambridge University Press:  05 March 2013

M. Meixner
M. Meixner*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. Email: meixner@stsci.edu
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Abstract

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We have performed a uniform and unbiased imaging survey of the Large Magellanic Cloud, using the IRAC and MIPS instruments on board the Spitzer Space Telescope. This Spitzer survey of the Large Magellanic Cloud is surveying the agents of a galaxy's evolution (SAGE), the interstellar medium and stars. The SAGE data are nonproprietary and the team has been creating catalogs and improved images for use by the astronomical community. This paper highlights some of the initial results being published by the SAGE team covering the topics of evolved stars and their mass-loss return to the ISM, young stellar objects and the properties of the ISM dust.

Keywords

Magellanic CloudsISM: duststars: circumstellar matterstars: formation
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 25 , Special Issue 3: The Magellanic System , 2008 , pp. 149 - 153
Copyright
Copyright © Astronomical Society of Australia 2008

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