Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?

Pavel Kroupa (), Hosein Haghi, Behnam Javanmardi, Akram Hasani Zonoozi, Oliver Müller, Indranil Banik, Xufen Wu, Hongsheng Zhao and Jörg Dabringhausen
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Pavel Kroupa: University of Bonn
Hosein Haghi: University of Bonn
Behnam Javanmardi: Institute for Research in Fundamental Sciences (IPM)
Akram Hasani Zonoozi: University of Bonn
Oliver Müller: Universität Basel
Indranil Banik: University of Saint Andrews
Xufen Wu: University of Science and Technology of China
Hongsheng Zhao: University of Saint Andrews
Jörg Dabringhausen: Faculty of Mathematics and Physics, Astronomical Institute

Nature, 2018, vol. 561, issue 7722, E4-E5

Keywords: Tidal Dwarf Galaxies; Globular Cluster Velocities; Surface Brightness Fluctuation Method; Velocity Dispersion; Primordial Dwarf (search for similar items in EconPapers)
Date: 2018
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DOI: 10.1038/s41586-018-0429-z

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