Abstract
The results of our study of a particular class of Galactic and extragalactic evolved stars, which are part of a binary system and surrounded by a stable dusty disc, are discussed. By combining spectroscopic, photometric and interferometric observations with detailed models describing dust properties and disc structure, we investigate the exact disc composition and structure.
Original language | English |
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Title of host publication | Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants |
Editors | Lebzelter, T. Wing, R.F. Kerschbaum, F. |
Place of Publication | San Francisco |
Publisher | Astronomical Society of the Pacific |
Pages | 309-313 |
Number of pages | 5 |
Publication status | Published - 2011 |