Does the galaxy NGC1052-DF2 falsify Milgromian dynamics?
Nature
.
2018 Sep;561(7722):E4-E5.
doi: 10.1038/s41586-018-0429-z.
Epub 2018 Sep 12.
Authors
Pavel Kroupa
1
2
,
Hosein Haghi
3
4
,
Behnam Javanmardi
5
,
Akram Hasani Zonoozi
3
4
,
Oliver Müller
6
,
Indranil Banik
7
,
Xufen Wu
8
9
,
Hongsheng Zhao
7
10
,
Jörg Dabringhausen
11
Affiliations
1
Helmholtz-Institut für Strahlen- und Kernphysik, University of Bonn, Bonn, Germany. pkroupa@uni-bonn.de.
2
Charles University in Prague, Faculty of Mathematics and Physics, Astronomical Institute, Prague, Czech Republic. pkroupa@uni-bonn.de.
3
Helmholtz-Institut für Strahlen- und Kernphysik, University of Bonn, Bonn, Germany.
4
Institute for Advanced Studies in Basic Sciences, Department of Physics, Zanjan, Iran.
5
School of Astronomy, Institute for Research in Fundamental Sciences (IPM), Tehran, Iran.
6
Departement Physik, Universität Basel, Basel, Switzerland.
7
Scottish Universities Physics Alliance, University of Saint Andrews, Saint Andrews, UK.
8
CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, China.
9
School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China.
10
Department of Physics and Astronomy, LaserLaB, Vrije Universiteit, Amsterdam, The Netherlands.
11
Charles University in Prague, Faculty of Mathematics and Physics, Astronomical Institute, Prague, Czech Republic.
PMID:
30209364
DOI:
10.1038/s41586-018-0429-z
No abstract available
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