THE EFFECT OF SUBLIMATION TEMPERATURE DEPENDENCIES ON DISK WALLS AROUND T TAURI STARS
The dust cannot survive closer to the star from the point where a grain reaches a temperature equal to the sublimation temperature. The boundary between a dust- free and a dusty region defines the sublimation wall. In the literature two models for the structure of the wall are used: a wall with a fi...
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| Veröffentlicht in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hauptverfasser: | , , , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Universidad Nacional Autónoma de México
2013
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| Schlagworte: | |
| Online-Zugang: | https://www.redalyc.org/articulo.oa?id=57126152005 |
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