A List of Groups of Dwarf Galaxies in the Local Supercluster
arXiv:1204.5406 · doi:10.1134/S1990341312020010
Abstract
We report a list of groups consisting of dwarf galaxies only. The sample contains 126 objects, mainly combined in pairs. The most populated group contains six dwarf galaxies. The majority of systems considered reside in the low-density regions and evolve unaffected by massive galaxies. The characteristic sizes and velocity dispersions of groups are 30 kpc and 11 km/s, respectively. They resemble the associations of dwarf galaxies, but are more compact. On the whole, groups and associations form a continuous sequence. Alike the associations, our groups possess high mass-to-luminosity ratios, what is indicative of a large amount of dark matter present in these systems.
17 pages, 6 figures, 2 tables, to be published in Astrophysical Bulletin 67, p.123 (2012)
References in corpus (8)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- CIRS: Cluster Infall Regions in the Sloan Digital Sky Survey I. Infall Patterns and Mass Profiles
- Near-Infrared and Optical Luminosity Functions from the 6dF Galaxy Survey
- The Hubble flow around the Local Group
- Binary Galaxies in the Local Supercluster and Its Neighborhood
- Catalog of Nearby Isolated Galaxies in the Volume z<0.01
- Cosmological Density Fluctuations on 100Mpc Scales and their ISW Effect
- Disturbed isolated galaxies: indicators of a dark galaxy population?
Cited by in corpus (15)
- Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
- Very high redshift quasars and the rapid emergence of super-massive black holes
- The KBC void and Hubble tension contradict CDM on a Gpc scale Milgromian dynamics as a possible solution
- A statistical investigation of the mass discrepancy-acceleration relation
- The failures of the standard model of cosmology require a new paradigm
- Cosmology and Convention
- Dynamics of astrophysical objects against the cosmological background
- Dark matter in galaxies
- Hubble flows and gravitational potentials in observable Universe
- Constraints on the star formation histories of galaxies in the Local Cosmological Volume
- Astrophysical Tests of Dark Matter Self-Interactions
- The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity
- Large-scale structure and galaxy motions in the Leo/Cancer constellations
- Enhanced prospects for direct detection of inelastic dark matter from a non-galactic diffuse component
- Gas of thin tubes of massless scalar field as a possible model of unified dark fluid