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- Rubin–Ford_effect abstract "The Rubin–Ford effect is the observation of a dipole anisotropy in the recessional velocity of a sample of ScI galaxies. This anisotropy is different in magnitude and direction from that of the cosmic microwave background radiation, and suggests that they are moving relative to the microwave background frame at about 800 km/s in the direction of the constellation Pegasus. It was found in 1976 by Vera Rubin and W. Kent Ford and became the subject of much discussion and interpretation over the following years.".
- Rubin–Ford_effect wikiPageExternalLink 1976AJ.....81..687R.
- Rubin–Ford_effect wikiPageExternalLink 1976AJ.....81..719R.
- Rubin–Ford_effect wikiPageID "12104224".
- Rubin–Ford_effect wikiPageLength "1074".
- Rubin–Ford_effect wikiPageOutDegree "11".
- Rubin–Ford_effect wikiPageRevisionID "648616850".
- Rubin–Ford_effect wikiPageWikiLink Category:Galaxy_morphological_types.
- Rubin–Ford_effect wikiPageWikiLink Category:Observational_astronomy.
- Rubin–Ford_effect wikiPageWikiLink Cosmic_microwave_background.
- Rubin–Ford_effect wikiPageWikiLink Dipole_anisotropy.
- Rubin–Ford_effect wikiPageWikiLink Galaxy.
- Rubin–Ford_effect wikiPageWikiLink Galaxy_morphological_classification.
- Rubin–Ford_effect wikiPageWikiLink Kent_Ford_(astronomer).
- Rubin–Ford_effect wikiPageWikiLink Pegasus_(constellation).
- Rubin–Ford_effect wikiPageWikiLink Recessional_velocity.
- Rubin–Ford_effect wikiPageWikiLink The_Astronomical_Journal.
- Rubin–Ford_effect wikiPageWikiLink Vera_Rubin.
- Rubin–Ford_effect wikiPageWikiLinkText "Rubin–Ford effect".
- Rubin–Ford_effect wikiPageUsesTemplate Template:Astronomy-stub.
- Rubin–Ford_effect subject Category:Galaxy_morphological_types.
- Rubin–Ford_effect subject Category:Observational_astronomy.
- Rubin–Ford_effect hypernym Observation.
- Rubin–Ford_effect type Aircraft.
- Rubin–Ford_effect type Type.
- Rubin–Ford_effect type Sub-discipline.
- Rubin–Ford_effect type Type.
- Rubin–Ford_effect comment "The Rubin–Ford effect is the observation of a dipole anisotropy in the recessional velocity of a sample of ScI galaxies. This anisotropy is different in magnitude and direction from that of the cosmic microwave background radiation, and suggests that they are moving relative to the microwave background frame at about 800 km/s in the direction of the constellation Pegasus. It was found in 1976 by Vera Rubin and W.".
- Rubin–Ford_effect label "Rubin–Ford effect".
- Rubin–Ford_effect sameAs Q7376126.
- Rubin–Ford_effect sameAs m.02vp_6x.
- Rubin–Ford_effect sameAs Q7376126.
- Rubin–Ford_effect wasDerivedFrom Rubin–Ford_effect?oldid=648616850.
- Rubin–Ford_effect isPrimaryTopicOf Rubin–Ford_effect.