Mass loss from red giants in the Magellanic Clouds

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The Magellanic Clouds provide the ideal laboratory for the study of mass loss and molecule and dust formation in red giants as a function of luminosity and metal abundance. I present some recent observational work.
Contribution to the proceedings of "The Spitzer Space Telescope: New Views of the Cosmos" (November 2004, Pasadena US). 2 pages, 1 figure

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