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Dwarf galaxies move in unexpected ways

Massive galaxies like our Milky Way are orbited by satellite dwarf galaxies. Standard cosmological simulations of galaxy formation predict that these satellites should move randomly around their host. Müller et al. examined the satellites of the nearby elliptical galaxy Centaurus A (see the Perspective by Boylan-Kolchin). They found that the satellites are distributed in a planar arrangement, and the members of the plane are orbiting in a coherent direction. This is inconsistent with more than 99% of comparable galaxies in simulations. Centaurus A, the Milky Way, and Andromeda all have highly statistically unlikely satellite systems. This observational evidence suggests that something is wrong with standard cosmological simulations.
Science, this issue p. 534; see also p. 520

Abstract

The Milky Way and Andromeda galaxies are each surrounded by a thin plane of satellite dwarf galaxies that may be corotating. Cosmological simulations predict that most satellite galaxy systems are close to isotropic with random motions, so those two well-studied systems are often interpreted as rare statistical outliers. We test this assumption using the kinematics of satellite galaxies around the Centaurus A galaxy. Our statistical analysis reveals evidence for corotation in a narrow plane: Of the 16 Centaurus A satellites with kinematic data, 14 follow a coherent velocity pattern aligned with the long axis of their spatial distribution. In standard cosmological simulations, <0.5% of Centaurus A–like systems show such behavior. Corotating satellite systems may be common in the universe, challenging small-scale structure formation in the prevailing cosmological paradigm.
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Supplementary Material

Summary

Materials and Methods
Supplementary Text
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Tables S1 and S2
References (5370)
Movie S1
Data Files S1 to S3

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Science
Volume 359Issue 63752 February 2018
Pages: 534 - 537

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Received: 24 June 2017
Accepted: 20 December 2017

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Departement Physik, Universität Basel, Klingelbergstrasse 82, CH-4056 Basel, Switzerland.
Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA.
Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia.
European Southern Observatory (ESO), Karl-Schwarschild-Strasse 1, 85748 Garching bei München, Germany.

Notes

*Corresponding author. Email: [email protected]

Funding Information

http://dx.doi.org/10.13039/501100000923Australian Research Council:
http://dx.doi.org/10.13039/501100001711Swiss National Science Foundation:

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Volume 359|Issue 6375
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