Linked from

The 61 pages that link to Dark matter halo, each with the reason it gives.

• Centaurus A/M83 GroupRelated: Invisible mass helps explain how galaxies remain bound within groups.

• Dark galaxyNarrower topic: Dark galaxies are proposed to occupy halos whose gas has not formed many stars.

• Field galaxyRelated: Halo mass and history can affect field galaxies independently of cluster membership.

• Galaxy rotation problemBroader topic: An extended halo supplies the extra gravitational pull used to explain flat rotation curves.

• Intergalactic starRelated: The cluster's halo governs the motions and distribution of many intergalactic stars.

• Jeans equationsRelated: Stellar velocity data analyzed with Jeans equations can constrain its mass profile.

• Messier 49Related: The motions of stars and globular clusters help constrain Messier 49’s halo.

• Unbarred spiral galaxyRelated: Its gravitational influence affects disk rotation and the growth of structure.

• Galaxy groups and clustersRelated: Most of a cluster’s mass lies in its extended dark matter halo.

• IC 342/Maffei GroupRelated: The group’s halo mass and extent are difficult to establish from its obscured galaxy census.

• Satellite galaxies of the Milky WayRelated: The Milky Way's halo supplies much of the gravity binding its satellites.