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      A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology

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          Abstract

          The Milky Way and Andromeda galaxy are each surrounded by a thin plane of satellite 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's satellites with kinematic data, 14 follow a coherent velocity pattern aligned with the long axis of their spatial distribution. In standard cosmology 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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          The observational case for a low-density Universe with a non-zero cosmological constant

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            Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

            We present the large-scale correlation function measured from a spectroscopic sample of 46,748 luminous red galaxies from the Sloan Digital Sky Survey. The survey region covers 0.72 h^{-3} Gpc^3 over 3816 square degrees and 0.16
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              Properties of galaxies reproduced by a hydrodynamic simulation

              Previous simulations of the growth of cosmic structures have broadly reproduced the 'cosmic web' of galaxies that we see in the Universe, but failed to create a mixed population of elliptical and spiral galaxies due to numerical inaccuracies and incomplete physical models. Moreover, because of computational constraints, they were unable to track the small scale evolution of gas and stars to the present epoch within a representative portion of the Universe. Here we report a simulation that starts 12 million years after the Big Bang, and traces 13 billion years of cosmic evolution with 12 billion resolution elements in a volume of \((106.5\,{\rm Mpc})^3\). It yields a reasonable population of ellipticals and spirals, reproduces the distribution of galaxies in clusters and statistics of hydrogen on large scales, and at the same time the metal and hydrogen content of galaxies on small scales.
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                Author and article information

                Journal
                31 January 2018
                Article
                10.1126/science.aao1858
                1802.00081
                ce59353e-5b9b-49f8-9065-605cca2302a2

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                Published in the first Feb 2018 issue of Science (M\"uller et al., Science 359, 534, 2018). This preprint corresponds to the accepted and language edited version of the manuscript. 32 pages, 5 figures
                astro-ph.GA astro-ph.CO

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