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Explaining The Mass Discrepancy In Galaxy Clusters
2017
Zenodo
Galaxy clusters and mass discrepancy blend and dwell together quite harmoniously. Mass discrepancy is always stumbled upon when galaxy clusters are studied. The orbital velocities of galaxies within galaxy clusters are unusually higher than expected and the observable baryonic matter alone cannot account for all the mass and gravity for the overall observed stability of the cluster. The presence of additional matter in the form of dark matter is required to explain the gravitational stability
doi:10.5281/zenodo.1003107
fatcat:jqc2pceywvguxfqxj7sdhxjtmy