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...
Na minha lista:
| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2002
|
| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57101313 |
| Tags: |
Ingen Tags, Vær først til at tagge denne postø!
|