GETTING TO GRIPS WITH THE UNKNOWN: HOW IMPORTANT ARE MAGNETIC FIELDS IN OUTFLOWS FROM YOUNG STARS?
Out ows are a ubiquitous part of the star formation process and may even be necessary if accretion is to occur onto a protostar or young brown dwarf. While an out ow can take several forms, it is most strikingly seen as a highly collimated supersonic jet that can stretch for several parsecs. Line em...
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Váldodahkki: | |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2009
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| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57115743026 |
| Fáddágilkorat: |
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