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- Q3356302 subject Q7215969.
- Q3356302 subject Q7446336.
- Q3356302 abstract "Galactic clusters are gravitationally bound large-scale structures of multiple galaxies. The evolution of these aggregates is determined by time and manner of formation and the process of how their structures and constituents have been changing with time. Gamow (1952) and Weizscker (1951) showed that the observed rotations of galaxies are important for cosmology. They postulated that the rotation of galaxies might be a clue of physical conditions under which these systems formed. Thus, understanding the distribution of spatial orientations of the spin vectors of galaxies is critical to understanding the origin of the angular momenta of galaxies.There are mainly three scenarios for the origin of galaxy clusters and superclusters. These models are based on different assumptions of the primordial conditions, so they predict different spin vector alignments of the galaxies. The three hypotheses are the pancake model, the hierarchy model, and the primordial vorticity theory. The three are mutually exclusive as they produce contradictory predictions. However, the predictions made by all three theories are based on the precepts of cosmology. Thus, these models can be tested using a database with appropriate methods of analysis.".
- Q3356302 wikiPageExternalLink 2006A%26A...458..357A.
- Q3356302 wikiPageExternalLink 2006MNRAS.366..438A.
- Q3356302 wikiPageExternalLink 2008MNRAS.389..741A.
- Q3356302 wikiPageWikiLink Q1536490.
- Q3356302 wikiPageWikiLink Q161254.
- Q3356302 wikiPageWikiLink Q184348.
- Q3356302 wikiPageWikiLink Q190397.
- Q3356302 wikiPageWikiLink Q2014003.
- Q3356302 wikiPageWikiLink Q204107.
- Q3356302 wikiPageWikiLink Q2121987.
- Q3356302 wikiPageWikiLink Q2488.
- Q3356302 wikiPageWikiLink Q27521.
- Q3356302 wikiPageWikiLink Q318.
- Q3356302 wikiPageWikiLink Q321.
- Q3356302 wikiPageWikiLink Q338.
- Q3356302 wikiPageWikiLink Q7215969.
- Q3356302 wikiPageWikiLink Q7446336.
- Q3356302 wikiPageWikiLink Q79925.
- Q3356302 wikiPageWikiLink Q854155.
- Q3356302 comment "Galactic clusters are gravitationally bound large-scale structures of multiple galaxies. The evolution of these aggregates is determined by time and manner of formation and the process of how their structures and constituents have been changing with time. Gamow (1952) and Weizscker (1951) showed that the observed rotations of galaxies are important for cosmology. They postulated that the rotation of galaxies might be a clue of physical conditions under which these systems formed.".
- Q3356302 label "Galactic orientation".