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Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?

Author

Listed:
  • Pavel Kroupa

    (University of Bonn
    Faculty of Mathematics and Physics, Astronomical Institute)

  • Hosein Haghi

    (University of Bonn
    Institute for Advanced Studies in Basic Sciences, Department of Physics)

  • Behnam Javanmardi

    (Institute for Research in Fundamental Sciences (IPM))

  • Akram Hasani Zonoozi

    (University of Bonn
    Institute for Advanced Studies in Basic Sciences, Department of Physics)

  • Oliver Müller

    (Universität Basel)

  • Indranil Banik

    (University of Saint Andrews)

  • Xufen Wu

    (University of Science and Technology of China
    University of Science and Technology of China)

  • Hongsheng Zhao

    (University of Saint Andrews
    LaserLaB, Vrije Universiteit)

  • Jörg Dabringhausen

    (Faculty of Mathematics and Physics, Astronomical Institute)

Abstract

No abstract is available for this item.

Suggested Citation

  • Pavel Kroupa & Hosein Haghi & Behnam Javanmardi & Akram Hasani Zonoozi & Oliver Müller & Indranil Banik & Xufen Wu & Hongsheng Zhao & Jörg Dabringhausen, 2018. "Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?," Nature, Nature, vol. 561(7722), pages 4-5, September.
    • Handle: RePEc:nat:nature:v:561:y:2018:i:7722:d:10.1038_s41586-018-0429-z
    DOI: 10.1038/s41586-018-0429-z
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