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- Bullet_Cluster abstract "The Bullet Cluster (1E 0657-558) consists of two colliding clusters of galaxies. Strictly speaking, the name Bullet Cluster refers to the smaller subcluster, moving away from the larger one. It is at a co-moving radial distance of 1.141 Gpc (3.721 Gly).Gravitational lensing studies of the Bullet Cluster are claimed to provide the best evidence to date for the existence of dark matter. At a statistical significance of 8σ, it was found that the spatial offset of the center of the total mass from the center of the baryonic mass peaks cannot be explained with an alteration of the gravitational force law. However, this interpretation of the gravitational lensing results is disputed, see below. Observations of other galaxy cluster collisions, such as MACS J0025.4-1222, also show significant displacement between their center of visible matter and their gravitational potential.".
- Bullet_Cluster thumbnail Bullet_cluster.jpg?width=300.
- Bullet_Cluster wikiPageExternalLink 0606216.
- Bullet_Cluster wikiPageExternalLink 0608407.
- Bullet_Cluster wikiPageExternalLink 0608408.
- Bullet_Cluster wikiPageExternalLink 0609125.
- Bullet_Cluster wikiPageExternalLink 0702146.
- Bullet_Cluster wikiPageExternalLink devil.
- Bullet_Cluster wikiPageExternalLink 1e0657.
- Bullet_Cluster wikiPageExternalLink bullet.mpg.
- Bullet_Cluster wikiPageExternalLink markevitch_maxim.pdf.
- Bullet_Cluster wikiPageExternalLink article.cfm?chanID=sa003&articleID=000EB9FD-823F-14EB-823F83414B7F0000.
- Bullet_Cluster wikiPageExternalLink 06-096.html.
- Bullet_Cluster wikiPageID "6487947".
- Bullet_Cluster wikiPageRevisionID "603747888".
- Bullet_Cluster caption "X-ray photo by Chandra X-ray Observatory. Exposure time was 140 hours. The scale is shown in megaparsecs. Redshift = 0.3, meaning its light has wavelengths stretched by a factor of 1.3.".
- Bullet_Cluster constellation Carina_(constellation).
- Bullet_Cluster distance ".".
- Bullet_Cluster distance "4000000000".
- Bullet_Cluster epoch Epoch_(astronomy).
- Bullet_Cluster flux "5.6".
- Bullet_Cluster hasPhotoCollection Bullet_Cluster.
- Bullet_Cluster luminosity "1.4".
- Bullet_Cluster name "Bullet Cluster".
- Bullet_Cluster otherNames "1".
- Bullet_Cluster redshift "0.296".
- Bullet_Cluster temperature "17.4".
- Bullet_Cluster subject Category:Carina_(constellation).
- Bullet_Cluster subject Category:Dark_matter.
- Bullet_Cluster subject Category:Galaxy_clusters.
- Bullet_Cluster type Abstraction100002137.
- Bullet_Cluster type Agglomeration107959269.
- Bullet_Cluster type Bunch107959943.
- Bullet_Cluster type Collection107951464.
- Bullet_Cluster type GalaxyClusters.
- Bullet_Cluster type Group100031264.
- Bullet_Cluster comment "The Bullet Cluster (1E 0657-558) consists of two colliding clusters of galaxies. Strictly speaking, the name Bullet Cluster refers to the smaller subcluster, moving away from the larger one. It is at a co-moving radial distance of 1.141 Gpc (3.721 Gly).Gravitational lensing studies of the Bullet Cluster are claimed to provide the best evidence to date for the existence of dark matter.".
- Bullet_Cluster label "1E 0657-558".
- Bullet_Cluster label "Amas du Boulet".
- Bullet_Cluster label "Bullet Cluster".
- Bullet_Cluster label "Bullet cluster".
- Bullet_Cluster label "Cúmulo Bala".
- Bullet_Cluster label "Gromada galaktyk 1E0657-558".
- Bullet_Cluster label "弾丸銀河団".
- Bullet_Cluster sameAs 1E_0657-558.
- Bullet_Cluster sameAs Cúmulo_Bala.
- Bullet_Cluster sameAs Amas_du_Boulet.
- Bullet_Cluster sameAs 弾丸銀河団.
- Bullet_Cluster sameAs 불릿_은하단.
- Bullet_Cluster sameAs Gromada_galaktyk_1E0657-558.
- Bullet_Cluster sameAs Bullet_cluster.
- Bullet_Cluster sameAs m.0g775t.
- Bullet_Cluster sameAs Q208935.
- Bullet_Cluster sameAs Q208935.
- Bullet_Cluster sameAs Bullet_Cluster.
- Bullet_Cluster wasDerivedFrom Bullet_Cluster?oldid=603747888.
- Bullet_Cluster depiction Bullet_cluster.jpg.
- Bullet_Cluster isPrimaryTopicOf Bullet_Cluster.