Mass loss from red giants in the Magellanic Clouds

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dc.creatorvan Loon, Jacco Th.
dc.date2005-03-02
dc.date.accessioned2026-07-07T02:17:07Z
dc.date.available2026-07-07T02:17:07Z
dc.descriptionThe 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.
dc.descriptionContribution to the proceedings of "The Spitzer Space Telescope: New Views of the Cosmos" (November 2004, Pasadena US). 2 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0503035
dc.identifierhttp://arxiv.org/abs/astro-ph/0503035
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9056
dc.subjectAstrophysics
dc.titleMass loss from red giants in the Magellanic Clouds
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