Exploring the central engines of young stars
If we are to understand the origins of emission line jets from young stars we have to probe their immediatecircumstellar environments on scales of 10AU or less. Although this is dicult to do in the case of highlyembedded stars, optically visible outow sources, such as classical T Tauri stars and Her...
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| 發表在: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
Universidad Nacional Autónoma de México
2002
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| 主題: | |
| 在線閱讀: | https://www.redalyc.org/articulo.oa?id=57101316 |
| 標簽: |
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