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A new yso outflow model, jet simulations, and their emission
In the usual theoretical picture of star formation a jet is ejected from a magnetized accretion disk, with amolecular outow being driven either by the jet or by a wider wind coming from the disk. We propose analternative unied model for the ows surrounding YSOs. In addition to a central accretion-ej...
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| Yayımlandı: | Revista Mexicana de Astronomía y Astrofísica |
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| Yazar: | |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
Universidad Nacional Autónoma de México
2002
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| Konular: | |
| Online Erişim: | https://www.redalyc.org/articulo.oa?id=57101313 |
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