A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
arXiv:1802.00081 · doi:10.1126/science.aao1858
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.
Published in the first Feb 2018 issue of Science (Müller et al., Science 359, 534, 2018). This preprint corresponds to the accepted and language edited version of the manuscript. 32 pages, 5 figures
References in corpus (20)
- Properties of galaxies reproduced by a hydrodynamic simulation
- Updated Nearby Galaxy Catalog
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- The Hubble flow around the CenA / M83 galaxy complex
- Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies
- From Tidal Dwarf Galaxies to Satellite Galaxies
- Two Planes of Satellites in the Centaurus A Group
- M31 Transverse Velocity and Local Group Mass from Satellite Kinematics
- Velocity anti-correlation of diametrically opposed galaxy satellites in the low redshift universe
- A thousand shadows of Andromeda: rotating planes of satellites in the Millennium-II cosmological simulation
- The Kinematics and Dynamics of the Globular Clusters and the Planetary Nebulae of NGC 5128
- Vast planes of satellites in a high resolution simulation of the Local Group: comparison to Andromeda
- A new spin on disks of satellite galaxies
- Testing the two planes of satellites in the Centaurus Group
- Chemo-dynamical evolution of tidal dwarf galaxies. II. The long-term evolution and influence of a tidal field
- VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies
- Eppur si muove: Positional and kinematic correlations of satellite pairs in the low Z universe
- The Centaurus Group and the Outer Halo of NGC 5128: Are they Dynamically Connected?
- NGC 5011C: an overlooked dwarf galaxy in the Centaurus A group
- An imaging and spectroscopic study of the planetary nebulae in NGC 5128 (Centaurus A): Planetary nebulae catalogues
Cited by in corpus (119)
- Direct Detection of WIMP Dark Matter: Concepts and Status
- The distribution of dark matter in galaxies
- Observational Evidence for Primordial Black Holes: A Positivist Perspective
- The large-scale structure of the halo of the Andromeda galaxy II. Hierarchical structure in the Pan-Andromeda Archaeological Survey
- An excess of small-scale gravitational lenses observed in galaxy clusters
- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- The Planes of Satellite Galaxies Problem, Suggested Solutions, and Open Questions
- Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies
- The Milky Way's Disk of Classical Satellite Galaxies in Light of Gaia DR2
- Limit on the LMC mass from a census of its satellites
- The KBC void and Hubble tension contradict CDM on a Gpc scale Milgromian dynamics as a possible solution
- The faint end of the Centaurus A satellite luminosity function
- The M101 Satellite Luminosity Function and the Halo to Halo Scatter Among Local Volume Hosts
- Wide-Field Survey of Dwarf Satellite Systems Around 10 Hosts in the Local Volume
- Dark matters on the scale of galaxies
- The dwarf galaxy satellite system of Centaurus A
- Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
- The Leo-I group: new dwarf galaxy and UDG candidates
- The Hubble Space Telescope Survey of M31 Satellite Galaxies I. RR Lyrae-based Distances and Refined 3D Geometric Structure
- Resolved Dwarf Galaxy Searches within ~5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam
- MOND simulation suggests the origin of some peculiarities in the Local Group
- Testing Gravity with wide binary stars like Centauri
- Ultra diffuse galaxies in the MATLAS low-to-moderate density fields
- The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology
- The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
- Metal-poor nuclear star clusters in two dwarf galaxies near Centaurus A suggesting formation from the in-spiraling of globular clusters
- Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
- Tracing satellite planes in the Sculptor group: I. Discovery of three faint dwarf galaxies around NGC 253
- Newly discovered dwarf galaxies in the MATLAS low density fields
- Evolution of galactic planes of satellites in the EAGLE simulation
- Origin of the Local Group satellite planes
- Galaxies lacking dark matter in the Illustris simulation
- Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Discovery of Three Ultra-faint Dwarf Galaxies
- The velocity anisotropy of the Milky Way satellite system
- Fuzzy Dark Matter at Cosmic Dawn: New 21-cm Constraints
- The Clustering of Orbital Poles Induced by the LMC: Hints for the Origin of Planes of Satellites
- Short Review of the main achievements of the Scalar Field, Fuzzy, Ultralight, Wave, BEC Dark Matter model
- The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure
- A Recent Major Merger Tale for the Closest Giant Elliptical Galaxy Centaurus A
- 3D hydrodynamic simulations for the formation of the Local Group satellite planes
- The formation of exponential disk galaxies in MOND
- Observational insights on the origin of giant low surface brightness galaxies
- Tip of the red giant branch distances to the dwarf galaxies dw1335-29 and dw1340-30 in the Centaurus group
- Mapping Dark Matter with Extragalactic Stellar Streams: the Case of Centaurus A
- Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. II.Observational constraints on the sub-galactic matter power spectrum
- Barred spiral galaxies in modified gravity theories
- Dwarf Galaxies in the Local Volume
- Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
- On the Co-Orbitation of Satellite Galaxies Along the Great Plane of Andromeda: NGC 147, NGC 185, and Expectations from Cosmological Simulations
- The properties of dwarf spheroidal galaxies in the Cen A group: Stellar populations, internal dynamics, and a heart-shaped Halpha ring
- The orientation of planes of dwarf galaxies in the quasi-linear Universe
- Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
- Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
- A Collection of New Dwarf Galaxies in NGC5128's Western Halo
- Radial velocities and stellar population properties of 56 MATLAS dwarf galaxies observed with MUSE
- The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
- Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
- Cosmological constraints on the Multi Scalar Field Dark Matter model
- An updated detailed characterization of planes of satellites in the MW and M31
- The PAndAS View of the Andromeda Satellite System. IV Global properties
- Galactic forces rule dynamics of Milky Way dwarf galaxies
- A stream come true: Connecting tidal tails, shells, streams, and planes with galaxy kinematics and formation history
- Planes of satellites around simulated disc galaxies: I.- Finding high-quality planar configurations from positional information and their comparison to MW/M31 data
- Study of gravitational fields and globular cluster systems of early-type galaxies
- A portrait of the Vast Polar Structure as a young phenomenon: hints from its member satellites
- On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies
- Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics
- The volume density of giant low surface brightness galaxies
- A correlation between the number of satellites and the baryonic bulge-to-total ratio extending beyond the Local Group
- The lopsided distribution of satellites of isolated central galaxies
- Faint Satellite Population of the NGC-3175 Group - a Local Group Analogue
- Sizing from the Smallest Scales: The Mass of the Milky Way
- The number of dwarf satellites of disk galaxies versus their bulge mass in the standard model of cosmology
- Scalar field dark matter as an alternative explanation for the anisotropic distribution of satellite galaxies
- The Origin of Lopsided Satellite Galaxy Distribution in Galaxy Pairs
- Consequences of the external field effect for MOND disk galaxies in galaxy clusters
- The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs
- The shape alignment of satellite galaxies in galaxy pairs in SDSS
- The imprint of galaxy mergers on satellite planes in a cosmological context
- Classifying the satellite plane membership of Centaurus A's dwarf galaxies using orbital alignment constraints
- Around the Spindle galaxy: the dark halo mass of NGC3115
- New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
- Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions
- On the absence of backsplash analogues to NGC 3109 in the CDM framework
- New dwarf galaxy candidates in the sphere of influence of the Sombrero galaxy
- Impact of distance determinations on Galactic structure. II. Old tracers
- Testing gravity with interstellar precursor missions
- Exploring the effects of primordial non-Gaussianity at galactic scales
- Tip of the red giant branch distance to the nearby dwarf galaxy [TT2009] 25 in the NGC 891 group
- Planes of satellites around simulated disk galaxies II: Time-persistent planes of kinematically-coherent satellites in CDM
- The spatial distribution of satellites in galaxy clusters
- New Velocity Measurements of NGC 5128 Globular Clusters out to 130 kpc: Outer Halo Kinematics, Substructure and Dynamics
- Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
- Lopsided distribution of MATLAS and ELVES dwarf satellite systems around isolated host galaxies
- Proper Motions of the Satellites of M31
- The quantum character of the Scalar Field Dark Matter
- Simulations of cluster ultra-diffuse galaxies in MOND
- Dark sector domain walls could explain the observed planes of satellites
- Sardinia Radio Telescope observations of Local Group dwarf galaxies -- I. The cases of NGC6822, IC1613, and WLM
- Shapes of dark matter haloes with discrete globular cluster dynamics: The example of NGC 5128 (Centaurus A)
- Dwarf Galaxies in the MATLAS Survey: The satellite system of NGC474 under scrutiny with MUSE
- IFUM Integrated Field Spectroscopy of Ten M104 Satellite Galaxy Candidates
- MUSE observations of dwarf galaxies and a stellar stream in the M83 group
- The Future of Dwarf Galaxy Research: What Telescopes Will Discover
- Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
- An LBT view of the co-rotating group of galaxies around NGC 2750: Deep imaging and new satellite candidates
- MOND-like behavior in the Dirac-Milne universe -- Flat rotation curves and mass/velocity relations in galaxies and clusters
- Tracing satellite planes in the Sculptor group: II. Discovery of five faint dwarf galaxies in the DESI Legacy Survey
- Effects of coplanar satellite bands on galactic disc evolution
- A Natural Explanation of the VPOS from Multistate Scalar Field Dark Matter
- MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites
- Testing a proposed "planarity" tool for studying satellite systems: On the alleged consistency of Milky Way satellite galaxy planes with CDM
- The Exploration of Local VolumE Satellites (ELVES) Survey: A Nearly Volume-Limited Sample of Nearby Dwarf Satellite Systems
- Are disks of satellites comprised of tidal dwarf galaxies?
- The Cen A galaxy group: dynamical mass and missing baryons
- The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models
- The Delegate Survey: KOALA/AAOmega-IFU spectroscopy of three nearby dwarf galaxies
- The long-term stability of the Vast Polar Structure and its connection to a possible previous passage of the LMC
- Implications of the correlation between bulge-to-total baryonic mass ratio and the number of satellites for SAGA galaxies