Disks Around Classical T Tauri Stars
We explain how observable properties of physically motivated models of accretion disks irradiated by their central stars can be compared with observations to quantify disk and dust properties. In particular, we discuss hints of dust evolution in disks around Classical T Tauri Stars.
Gardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autor Principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2003
|
| Assuntos: | |
| Acceso en liña: | https://www.redalyc.org/articulo.oa?id=57101806 |
| Tags: |
Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!
|