Resolved images of a protostellar outflow driven by an extended disk wind

Per Bjerkeli (), Matthijs H. D. van der Wiel, Daniel Harsono, Jon P. Ramsey and Jes K. Jørgensen
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Per Bjerkeli: Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen
Matthijs H. D. van der Wiel: Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen
Daniel Harsono: Center for Astronomy, Institute of Theoretical Astrophysics, Heidelberg University
Jon P. Ramsey: Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen
Jes K. Jørgensen: Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen

Nature, 2016, vol. 540, issue 7633, 406-409

Abstract: Observations of the outflow associated with the TMC1A protostellar system reveal that the ‘disk wind’ model correctly explains how material is ejected from protostars.

Date: 2016
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DOI: 10.1038/nature20600

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