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

Author

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  • Per Bjerkeli

    (Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen
    Chalmers University of Technology, Onsala Space Observatory)

  • Matthijs H. D. van der Wiel

    (Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen
    ASTRON, the Netherlands Institute for Radio Astronomy)

  • 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)

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.

Suggested Citation

  • Per Bjerkeli & Matthijs H. D. van der Wiel & Daniel Harsono & Jon P. Ramsey & Jes K. Jørgensen, 2016. "Resolved images of a protostellar outflow driven by an extended disk wind," Nature, Nature, vol. 540(7633), pages 406-409, December.
    • Handle: RePEc:nat:nature:v:540:y:2016:i:7633:d:10.1038_nature20600
    DOI: 10.1038/nature20600
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