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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Bibliographic Details
Main Authors:	Bjerkeli, Per (Author) , Wiel, Matthijs H. D. van der (Author) , Harsono, Daniel (Author) , Ramsey, Jon P. (Author) , Jorgensen, Jes K. (Author)
Format:	Article (Journal)
Language:	English
Published:	14 December 2016
In:	Nature Year: 2016, Volume: 540, Issue: 7633, Pages: 406-409
ISSN:	1476-4687
DOI:	10.1038/nature20600
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1038/nature20600 Verlag, lizenzpflichtig, Volltext: https://www.nature.com/articles/nature20600
Author Notes:	Per Bjerkeli, Matthijs H. D. van der Wiel, Daniel Harsono, Jon P. Ramsey, & Jes K. Jørgensen

Description
Summary:	Observations of the outflow associated with the TMC1A protostellar system reveal that the ‘disk wind’ model correctly explains how material is ejected from protostars.
Item Description:	Gesehen am 13.05.2020
Physical Description:	Online Resource
ISSN:	1476-4687
DOI:	10.1038/nature20600