Cosmicflows-3: Cosmography of the Local Void
arXiv:1905.08329 · doi:10.3847/1538-4357/ab2597
Abstract
Cosmicflows-3 distances and inferred peculiar velocities of galaxies have permitted the reconstruction of the structure of over and under densities within the volume extending to 0.05c. This study focuses on the under dense regions, particularly the Local Void that lies largely in the zone of obscuration and consequently has received limited attention. Major over dense structures that bound the Local Void are the Perseus-Pisces and Norma-Pavo-Indus filaments separated by 8,500 km/s. The void network of the universe is interconnected and void passages are found from the Local Void to the adjacent very large Hercules and Sculptor voids. Minor filaments course through voids. A particularly interesting example connects the Virgo and Perseus clusters, with several substantial galaxies found along the chain in the depths of the Local Void. The Local Void has a substantial dynamical effect, causing a deviant motion of the Local Group of 200-250 km/s. The combined perturbations due to repulsion from the Local Void and attraction toward the Virgo Cluster account for about 50% of the motion of the Local Group in the rest frame given by the cosmic microwave background.
arXiv comment18 pages; 9 figures; links to 1 video and 2 interactive models
References in corpus (29)
- How Filaments are Woven into the Cosmic Web
- Cosmicflows-3
- The Laniakea supercluster of galaxies
- Wiener Reconstruction of The Large Scale Structure
- A kinematic classification of the cosmic web
- Wiener Reconstruction of Large-Scale Structure from Peculiar Velocities
- Cosmography of the Local Universe
- Action Principle Solutions For Galaxy Motions Within 3000 Km/s
- Action Dynamics of the Local Supercluster
- 3D Velocity and Density Reconstructions of the Local Universe with Cosmicflows-1
- The peculiar velocity field up to by forward-modeling Cosmicflows-3 data
- Detection of a Supervoid Aligned with the Cold Spot of the Cosmic Microwave Background
- The Dipole Repeller
- The Formation of the Local Group Planes of Galaxies
- A Robust Tip of the Red Giant Branch Distance to the Fireworks Galaxy (NGC 6946)
- Constrained Local UniversE Simulations: A Local Group Factory
- Midlife Crises in Dwarf Galaxies in the NGC 5353/4 Group
- Supervoids in the WISE-2MASS catalogue imprinting Cold Spots in the Cosmic Microwave Background
- Bayesian 3d velocity field reconstruction with VIRBIuS
- Cosmic troublemakers: the Cold Spot, the Eridanus Supervoid, and the Great Walls
- Pecular velocities of galaxies in the Leo Spur
- Void galaxies in the nearby Universe. I. Sample description
- Cosmicflows-3: Cold Spot Repeller?
- The quasi-linear nearby Universe
- The Cosmic V-Web
- The Arrowhead Mini-Supercluster of Galaxies
- Draining the Local Void
- Low-Density Structures in the Local Universe. II. Nearby Cosmic Voids
- The Distance and Motion of the Maffei Group
Cited by in corpus (48)
- Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances
- The Hestia project: simulations of the Local Group
- Using The Baryonic Tully-Fisher Relation to Measure
- Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
- The Extragalactic Distance Database: The Color-Magnitude Diagrams and Tip of the Red Giant Branch Distances Catalog
- Cosmicflows-3: Two DistanceVelocity Calculators
- Toward determining the number of observable supermassive black hole shadows
- Observational evidence for a local underdensity in the Universe and its effect on the measurement of the Hubble Constant
- Virgo Filaments I: Processing of gas in cosmological filaments around the Virgo cluster
- Testing the Strong Equivalence Principle. II. Relating the External Field Effect in Galaxy Rotation Curves to the Large-Scale Structure of the Universe
- MIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years
- Early Science from POSSUM: Shocks, turbulence, and a massive new reservoir of ionised gas in the Fornax cluster
- The 2MASS redshift survey galaxy group catalogue derived from a graph-theory based friends-of-friends algorithm
- Cosmicflows-3: The South Pole Wall
- The orientation of planes of dwarf galaxies in the quasi-linear Universe
- Evidence of ram pressure stripping of WLM, a dwarf galaxy far away from any large host galaxy
- Bulk Flow Motion Detection in the Local Universe with Pantheon Type Ia Supernovae
- The Warm Gas in the MW: A Kinematical Model
- Probing cosmic isotropy in the Local Universe
- Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
- WALLABY Pre-Pilot and Pilot Survey: the Tully Fisher Relation in Eridanus, Hydra, Norma and NGC4636 fields
- WALLABY pre-pilot survey: Two dark clouds in the vicinity of NGC 1395
- Cosmology in Minkowski space
- The Cosmic Large-Scale Structure in X-rays (CLASSIX) cluster survey IV: Superclusters in the local Universe at z <= 0.03
- HI Galaxy Signatures in the SARAO MeerKAT Galactic Plane Survey -- II. The Local Void and its substructure
- Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
- Constrained cosmological simulations of the Local Group using Bayesian hierarchical field-level inference
- The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey III: The Perseus-Pisces supercluster and the Southern Great Wall as traced by X-ray luminous galaxy clusters
- On the Merger Rate of Primordial Black Holes in Cosmic Voids
- Machine-learning computation of distance modulus for local galaxies
- Galaxy flows within 8,000 km/s from Numerical Action methods
- AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
- Testing Bayesian reconstruction methods from peculiar velocities
- Anomalous Stellar Populations in LSB Galaxies
- KKH 22, the first dwarf spheroidal satellite of IC 342
- MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at
- Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
- The Distance and Peculiar Velocity of the Norma cluster (ACO 3627) using the Near-Infrared and -band Fundamental Plane Relations
- On the convergence of cosmographic expansions in Lemaitre-Tolman-Bondi models
- Toward Cosmicflows-4: The \hi data catalog
- Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
- Infall of galaxies onto groups
- Cosmology with Cosmic Voids
- Chemodynamic evidence of pristine gas accretion in the void galaxy VGS 12
- Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
- AVISM: Algorithm for Void Identification in coSMology
- Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
- The effects of lensing by local structures on the dipole of radio source counts