Circumstellar Dust around M, S and C Stars
| Autor: | Irene R. Little-Marenin |
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| Rok vydání: | 2000 |
| Předmět: | |
| Zdroj: | Symposium - International Astronomical Union. 177:361-366 |
| ISSN: | 0074-1809 |
| DOI: | 10.1017/s0074180900002606 |
| Popis: | The circumstellar shells of M stars produce emission features due to amorphous silicates peaking around 10 and 18 μm, with additional emission at 11 μm due to crystalline olivine and at 13.1 μm (unknown carrier). C stars are associated with SiC dust emission at 11.2 μm with additional emission around 8.9 μm, whereas S stars have a relatively weak 10.5 μm emission feature which is due neither to silicates nor to SiC. |
| Databáze: | OpenAIRE |
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