The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
arXiv:2208.02265 · doi:10.1093/mnras/stac1765
Abstract
Due to their low surface brightness, dwarf galaxies are particularly susceptible to tidal forces. The expected degree of disturbance depends on the assumed gravity law and whether they have a dominant dark halo. This makes dwarf galaxies useful for testing different gravity models. In this project, we use the Fornax Deep Survey (FDS) dwarf galaxy catalogue to compare the properties of dwarf galaxies in the Fornax Cluster with those predicted by the Lambda cold dark matter (CDM) standard model of cosmology and Milgromian dynamics (MOND). We construct a test particle simulation of the Fornax system. We then use the MCMC method to fit this to the FDS distribution of tidal susceptibility (half-mass radius divided by theoretical tidal radius), the fraction of dwarfs that visually appear disturbed as a function of , and the distribution of projected separation from the cluster centre. This allows us to constrain the value at which dwarfs should get destroyed by tides. Accounting for an -band surface brightness limit of 27.8 magnitudes per square arcsec, the required stability threshold is in CDM and in MOND. The CDM value is in tension with previous -body dwarf galaxy simulations, which indicate that . Our MOND -body simulations indicate that , which agrees well with our MCMC analysis of the FDS. We therefore conclude that the observed deformations of dwarf galaxies in the Fornax Cluster and the lack of low surface brightness dwarfs towards its centre are incompatible with CDM expectations but well consistent with MOND.
35 pages, 24 figures, 4 tables, 7.5 MB. Accepted for publication in Monthly Notices of the Royal Astronomical Society in this form, first figure caption and equation 65 fixed, references updated
References in corpus (66)
- A direct empirical proof of the existence of dark matter
- Ultralight scalars as cosmological dark matter
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue
- The Tidal Evolution of Local Group Dwarf Spheroidals
- One Law To Rule Them All: The Radial Acceleration Relation of Galaxies
- Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest
- Disruption of Dark Matter Substructure: Fact or Fiction?
- A new relativistic theory for Modified Newtonian Dynamics
- On the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos
- Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies
- Two Planes of Satellites in the Centaurus A Group
- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- THINGS about MOND
- 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
- The KBC void and Hubble tension contradict CDM on a Gpc scale Milgromian dynamics as a possible solution
- Are sterile neutrinos consistent with clusters, the CMB and MOND?
- A thousand shadows of Andromeda: rotating planes of satellites in the Millennium-II cosmological simulation
- The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies
- Dense Stellar Populations: Initial Conditions
- Gaia EDR3 proper motions of Milky Way dwarfs I: 3D Motions and Orbits
- Fast galaxy bars continue to challenge standard cosmology
- Phantom of RAMSES (POR): A new Milgromian dynamics N-body code
- The Fornax Deep Survey (FDS) with VST. VI. Optical properties of the dwarf galaxies in the Fornax cluster
- Andromeda Dwarfs in Light of MOND
- A massive blow for CDM the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
- Stellar Kinematics and Structural Properties of Virgo Cluster Dwarf Early-Type Galaxies from the SMAKCED Project II. The Survey and a Systematic Analysis of Kinematic Anomalies and Asymmetries
- Galaxies lacking dark matter produced by close encounters in a cosmological simulation
- The Equilibrium Temperature of Planets in Elliptical Orbits
- The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology
- Tidal dwarf galaxies in cosmological simulations
- The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps
- Star formation triggered by galaxy interactions in modified gravity
- Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
- A blind ATCA HI survey of the Fornax galaxy cluster: properties of the HI detections
- A new formulation of the external field effect in MOND and numerical simulations of ultra-diffuse dwarf galaxies application to NGC 1052-DF2 and NGC 1052-DF4
- Testing the Strong Equivalence Principle. II. Relating the External Field Effect in Galaxy Rotation Curves to the Large-Scale Structure of the Universe
- Statistical significance of the sterile-neutrino hypothesis in the context of reactor and gallium data
- Structure and kinematics of tidally limited satellite galaxies in LCDM
- Stellar streams as gravitational experiments II. Asymmetric tails of globular cluster streams
- The Carnegie Chicago Hubble Program X: Tip of the Red Giant Branch Distances to NGC 5643 and NGC 1404
- Orbital evidences for dark-matter-free Milky Way dwarf spheroidal galaxies
- The global stability of M33: still a puzzle
- The formation of exponential disk galaxies in MOND
- 3D hydrodynamic simulations for the formation of the Local Group satellite planes
- The global stability of M33 in MOND
- And In The Darkness Unbind Them: High-Resolution Simulations of Dark Matter Subhalo Disruption in a Milky Way-like Tidal Field
- Barred spiral galaxies in modified gravity theories
- On the Co-Orbitation of Satellite Galaxies Along the Great Plane of Andromeda: NGC 147, NGC 185, and Expectations from Cosmological Simulations
- Probing the radial acceleration relation and the strong equivalence principle with the Coma cluster ultra-diffuse galaxies
- Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
- The Milky Way's rotation curve with superfluid dark matter
- The Phantom of RAMSES user guide for galaxy simulations using Milgromian and Newtonian gravity
- The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
- Discussing the first velocity dispersion profile of an ultra-diffuse galaxy in MOND
- Heat capacity of Holographic screen inspires MOND theory
- Lopsidedness of self-consistent galaxies by the external field effect of clusters
- On the absence of backsplash analogues to NGC 3109 in the CDM framework
- Galactic Mass-to-Light Ratios With Superfluid Dark Matter
- Deep-MOND polytropes
- Galactic tides and the Crater II dwarf spheroidal: a challenge to LCDM?
- The Baryonic Tully-Fisher Relation in the Local Group and the Equivalent Circular Velocity of Pressure Supported Dwarfs
- The Fornax Deep Survey (FDS) with the VST: III. Low Surface Brightness (LSB) dwarfs and Ultra Diffuse Galaxies (UDGs) in the center of the Fornax cluster
- Overestimated inclinations of Milgromian disc galaxies: the case of the ultradiffuse galaxy AGC 114905
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- Strong constraints on the gravitational law from DR3 wide binaries
- Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah challenge Newtonian gravitation
- Models of modified-inertia formulation of MOND
- Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
- On the tension between the Radial Acceleration Relation and Solar System quadrupole in modified gravity MOND
- A co-rotating gas and satellite structure around the interacting galaxy pair NGC 4490/85
- Simulations of star forming main sequence galaxies in Milgromian gravity
- Hydrodynamical structure formation in Milgromian cosmology
- The SAMI -- Fornax Dwarfs Survey II: The Stellar Mass Fundamental Plane and the Dark Matter fraction of Dwarf Galaxies
- Open star clusters and their asymmetrical tidal tails
- The impact of environment on size: Galaxies are 50% smaller in the Fornax Cluster compared to the field
- MOND as a peculiar case of the SIV theory
- A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
- The Magellanic Clouds are very rare in the IllustrisTNG simulations
- Galaxy rotation curve in hyperconical universes: a natural relativistic MOND
- SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
- Dynamical friction in the quasi-linear formulation of modified Newtonian dynamics (QuMOND)
- Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
- Simulations of cluster ultra-diffuse galaxies in MOND
- Velocity dispersion of dark matter deficient ultra-diffuse galaxies: A case for modified gravity
- A Relativistic Scalar Model for Fractional Interaction between Dark Matter and Gravity
- Asymmetry at Low Surface Brightness as an Indicator of Environmental Processes in the Fornax Cluster
- Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
- Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
- Fast particle-mesh code for Milgromian dynamics
- Hydrostatic equilibrium of X-ray gas in X-COP clusters with HMG
- Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
- On the Evidence for Violation of the Equivalence Principle in Disk Galaxies
- The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models