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References
van Dokkum, P. et al. A galaxy lacking dark matter. Nature 555, 629–632 (2018).
Milgrom, M. A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis. Astrophys. J. 270, 365–370 (1983).
Famaey, B. & McGaugh, S. S. Modified Newtonian dynamics (MOND): observational phenomenology and relativistic extensions. Living Rev. Relativ. 15, 10 (2012).
Haghi, H. et al. Testing fundamental physics with distant star clusters: theoretical models for pressure-supported stellar systems. Mon. Not. R. Astron. Soc. 395, 1549–1557 (2009).
Ploeckinger, S. et al. Tidal dwarf galaxies in cosmological simulations. Mon. Not. R. Astron. Soc. 474, 580–596 (2018).
Bekenstein, J. & Milgrom, M. Does the missing mass problem signal the breakdown of Newtonian gravity? Astrophys. J. 286, 7–14 (1984).
Kroupa, P. The dark matter crisis: falsification of the current standard model of cosmology. Publ. Astron. Soc. Aust. 29, 395–433 (2012).
Milgrom, M. The modified dynamics as a vacuum effect. Phys. Lett. A 253, 273–279 (1999).
Milgrom, M. Solutions for the modified Newtonian dynamics field equation. Astrophys. J. 302, 617–625 (1986).
McGaugh, S. S. MOND prediction for the velocity dispersion of the “feeble giant” Crater II. Astrophys. J. 832, L8 (2016).
Thomas, G. F. et al. Stellar streams as gravitational experiments. II. Asymmetric tails of globular cluster streams. Astron. Astrophys. 609, A44 (2018).
Beers, T. C., Flynn, K. & Gebhardt, K. Measures of location and scale for velocities in clusters of galaxies - a robust approach. Astron. J. 100, 32–46 (1990).
Fernández-Ontiveros, J. A., López-Sanjuan, C., Montes, M., Prieto, M. A. & Acosta-Pulido, J. A. The most recent burst of star formation in the massive elliptical galaxy NGC 1052. Mon. Not. R. Astron. Soc. 411, L21–L25 (2011).
Bellstedt, S. et al. The SLUGGS survey: a comparison of total-mass profiles of early type galaxies from observations and cosmological simulations, to 4 effective radii. Mon. Not. R. Astron. Soc. 476, 4543–4564 (2018).
Londrillo, P. & Nipoti, C. N-MODY: a code for collisionless N-body simulations in modified Newtonian dynamics. Mem. Soc. Astron. Ital. Suppl. 13, 89 (2009).
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P.K. conceived the work and wrote the manuscript; H.H. and A.H.Z. performed the external field effect calculations; O.M. and B.J. contributed observational expertise on galaxies; I.B., X.W. and H.Z. contributed MOND expertise; J.D. contributed dwarf galaxy expertise. All co-authors contributed to the manuscript with comments and passages.
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This file contains the external field effect calculation in MOND
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Kroupa, P., Haghi, H., Javanmardi, B. et al. Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?. Nature 561, E4–E5 (2018). https://doi.org/10.1038/s41586-018-0429-z
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DOI: https://doi.org/10.1038/s41586-018-0429-z
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