Resolved images of a protostellar outflow driven by an extended disk wind
Observations of the outflow associated with the TMC1A protostellar system reveal that the ‘disk wind’ model correctly explains how material is ejected from protostars.
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| Hauptverfasser: | , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
14 December 2016
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| In: |
Nature
Year: 2016, Jahrgang: 540, Heft: 7633, Pages: 406-409 |
| ISSN: | 1476-4687 |
| DOI: | 10.1038/nature20600 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1038/nature20600 Verlag, lizenzpflichtig, Volltext: https://www.nature.com/articles/nature20600 
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| Verfasserangaben: | Per Bjerkeli, Matthijs H. D. van der Wiel, Daniel Harsono, Jon P. Ramsey, & Jes K. Jørgensen |
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