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.
Cite
@article{arxiv.astro-ph/0503035,
title = {Mass loss from red giants in the Magellanic Clouds},
author = {Jacco Th. van Loon},
journal= {arXiv preprint arXiv:astro-ph/0503035},
year = {2007}
}
Comments
Contribution to the proceedings of "The Spitzer Space Telescope: New Views of the Cosmos" (November 2004, Pasadena US). 2 pages, 1 figure