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| Format: | Artículo científico |
| Langue: | en |
| Publié: |
Universidad Nacional Autónoma de México
2002
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| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57101313 |
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Table des matières:
- A new yso outflow model, jet simulations, and their emission T. Lery Física, Astronomía y Matemáticas MAIN SEQUENCE STARS: PRE MAGNETOHYDRODYNAMICS ISM: JETS AND OUTFLOWS 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-ejection enginedriving the jet, the molecular outow is powered by the infalling matter and follows a circulation pattern aroundthe central object without being entrained by an outow. Jets solutions from this model have been used asinitial conditions for simulations of the propagation of pulsed jets. Synthetic maps from the jet simulations arepresented. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101313 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.13