A parsec-scale optical jet from a massive young star in the Large Magellanic Cloud
Anna F. McLeod (),
Megan Reiter,
Rolf Kuiper,
Pamela D. Klaassen and
Christopher J. Evans
Additional contact information
Anna F. McLeod: School of Physical and Chemical Sciences, University of Canterbury
Megan Reiter: University of Michigan
Rolf Kuiper: Institute of Astronomy and Astrophysics, University of Tübingen
Pamela D. Klaassen: UK Astronomy Technology Centre, Royal Observatory Edinburgh
Christopher J. Evans: UK Astronomy Technology Centre, Royal Observatory Edinburgh
Nature, 2018, vol. 554, issue 7692, 334-336
Abstract:
Observations of a highly collimated, parsec-scale jet emitted from a massive young stellar object in the Large Magellanic Cloud indicate that jet launching and collimation are independent of stellar mass.
Date: 2018
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Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:554:y:2018:i:7692:d:10.1038_nature25189
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DOI: 10.1038/nature25189
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