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• The Motion of Clusters of Galaxies
  | title = The Motion of Clusters of Galaxies | keywords = [[Galaxy Clusters]]
  358 bytes (37 words) - 20:04, 1 January 2017
• High Redshift Galaxies May be Clusters of Galaxies
  | title = High Redshift Galaxies May be Clusters of Galaxies | keywords = [[galaxy clusters]], [[big bang cosmology]], [[tired light]]
  1,004 bytes (139 words) - 19:36, 1 January 2017
• Continuum Theory (CT): its particle-tied aether yields a Continuous Auto-Creation (CAC) cosmology with no Big Bang; with implication for stellar metallicity and for understanding the construction and morphological evolution of galaxies and clusters
  ...understanding the construction and morphological evolution of galaxies and clusters ...ic redshift]], [[no BigBang]], [[continuous-creation cosmology]], [[galaxy clusters]]
  2 KB (224 words) - 19:24, 1 January 2017
• On the Visual Images that Galaxies Create
  ...ads to a spiral shaped background field that the normal sized stars of the galaxy fall into, thereby creating the spiral appearance. I first began writing ab
  2 KB (288 words) - 19:48, 1 January 2017
• Kozyrev?s Causal Mechanics in Stellar Systems: Predictions and Estimations
  ...erties of stellar systems. Some qualitative features of galaxy groups and clusters in the presence of quasars and active galactic nuclei are predicted from th
  777 bytes (98 words) - 10:36, 1 January 2017
• Miles F Osmaston
  | known_for = [[Fundamental nature of gravitation; cosmic physics; galaxy & planet formation and evolution; mantle properties & plate tectonics mecha ...understanding the construction and morphological evolution of galaxies and clusters]]" ([http://www.naturalphilosophy.org/pdf/abstracts/abstracts_6805.pdf Read
  2 KB (245 words) - 13:04, 30 December 2016
• Interacting galaxy
  ...mple of a major interaction is a galactic collision, which may lead to a [[galaxy merger]]. ...le=HubbleSite: News - Hubble Finds that "Blue Blobs" in Space Are Orphaned Clusters of Stars|website=hubblesite.org|access-date=2017-05-24}}</ref>
  12 KB (1,640 words) - 19:51, 4 February 2018
• David G Russell
  ...determination of the Hubble parameter from 218 ScI galaxies and 16 galaxy clusters" ''Journal of Astrophysics &amp; Astronomy'' (August 2009). From 2000 to th
  1 KB (200 words) - 12:36, 30 December 2016
• A Survey of Anomalous Redshifts
  ...ctively, D. G. Russell, M. Lopez-Corredoira, and H. C. Arp, and for galaxy clusters and large-scale structures, those of N. A. Bahcall5, J.C. Jackson, and N. K
  2 KB (241 words) - 19:20, 1 January 2017
• Relativistic Reality: A Modern View (Knots and Everything, Vol 12)
  ...<tr> <td> <div class="tockeyword">galaxy clusters, geodesic, closed universe </div></td> </tr>...
  15 KB (2,010 words) - 06:46, 2 January 2017
• Arp 220
  {{Infobox Galaxy | image = [[Image:Galaxy arp 220.jpg|250px|]]
  7 KB (1,006 words) - 12:34, 5 February 2018
• A Modified Law of Gravitation taking Account of the Relative Speeds of Moving Masses A Preliminary Study
  ...of the Pioneer satellites, that of stars in galaxies or galaxies in galaxy clusters, for the same value of one additional parameter. The law equally simulates
  2 KB (322 words) - 18:25, 29 December 2016
• A Modified Law of Gravitation taking Account of the Relative Speeds of Moving Masses. A Preliminary Study
  ...of the Pioneer satellites, that of stars in galaxies or galaxies in galaxy clusters, for the same value of one additional parameter. The law equally simulates
  2 KB (344 words) - 19:16, 1 January 2017
• Gravitomagnetism - Gravity beyond Einstein - including an introduction to the Coriolis Gravity Theory
  ...got so few windings around the centre, in spite of the elevated age of the galaxy. Moreover we will discover the reason for the shape of the remnants of some
  4 KB (622 words) - 06:39, 2 January 2017
• VES Theory and the Forces of Nature
  ...f gravitation, it too appears to have elastic properties. In our Milky Way Galaxy, as well as other galaxies, the farther a star is from the galactic center ...r the influenced of their own internal gravity, but not attracted to other clusters at greater distance.
  7 KB (1,117 words) - 06:56, 2 January 2017
• Big Bang Reaches Deflation Stage
  ...the "SZ effect" showing heating of the radiation by x-rays in some galaxy clusters now shows cooling in roughly half the cases, consistent with random fluctua
  4 KB (600 words) - 19:21, 1 January 2017
• Centaurus A
  {{Infobox galaxy | title=The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances
  29 KB (4,015 words) - 12:30, 5 February 2018
• Redshift quantization
  ...ue=2 |pages=802 |bibcode=2001ApJ...549..802A |doi=10.1086/319438|quote=The clusters and the galaxies in them tend to be strong X-ray and radio emitters, and th ...uantization in excess of what is expected due to [[selection effect]] or [[galaxy cluster|galactic clustering]].<ref>{{cite journal |last1=Trimble |first1=V.
  22 KB (3,040 words) - 20:16, 4 February 2018
• Atlas of Peculiar Galaxies
  [[Image:Arp87full.jpg|thumb|300px|Colliding [[spiral galaxy]] pair [[NGC 3808]]A and NGC 3808B (Arp 87).]] ...24).jpg|thumb|300px|[[NGC 6621]]/[[NGC 6622]] (Arp 81), a pair of [[spiral galaxy|spiral galaxies]] 100 million years after their colliding.]]
  76 KB (10,108 words) - 13:04, 4 February 2018
• Halton Arp
  ...38 nearby galaxies that did not fall into any of the classic categories of galaxy shapes. His goal was to produce a selection that modellers could use in ord ...esis]] is that quasars are local objects ejected from the core of [[Active galaxy|active galactic nuclei]] (AGN). Nearby galaxies with both strong radio emis
  19 KB (2,646 words) - 14:44, 2 August 2020

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