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The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3

Author

Listed:
  • R. J. Wilman

    (University of Durham)

  • J. Gerssen

    (University of Durham)

  • R. G. Bower

    (University of Durham)

  • S. L. Morris

    (University of Durham)

  • R. Bacon

    (CRAL-Observatoire)

  • P. T. de Zeeuw

    (Leiden Observatory)

  • R. L. Davies

    (Astrophysics, University of Oxford)

Abstract

Gas leak Galaxy formation is thought to involve the cooling of gas in dark-matter haloes collapsing under the influence of gravity and the expansion of the Universe. Cosmologists have a problem with this model though: it produces too many bright galaxies. Unless, that is, young galaxies eject large amounts of gas in the form of high-speed outflows. A new technique, integral field spectroscopy has now been used to gather the best evidence yet that such processes actually occur.

Suggested Citation

  • R. J. Wilman & J. Gerssen & R. G. Bower & S. L. Morris & R. Bacon & P. T. de Zeeuw & R. L. Davies, 2005. "The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3," Nature, Nature, vol. 436(7048), pages 227-229, July.
    • Handle: RePEc:nat:nature:v:436:y:2005:i:7048:d:10.1038_nature03718
    DOI: 10.1038/nature03718
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