Results 141 to 150 of about 173,637 (267)
The Impact of Galaxy-halo Size Relations on Galaxy Clustering Signals
Galaxies come in different sizes and morphologies, and these differences are thought to correlate with properties of their underlying dark matter halos.
Joshua B. Hill, Yao-Yuan Mao
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BEC dark matter can explain collisions of galaxy clusters [PDF]
Jae-Weon Lee, Sooil Lim, Dale Choi
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Erratum: “Formation and Evolution of Galaxy Dark Matter Halos and Their Substructure” (ApJ, 667, 859 [2007]) [PDF]
Jürg Diemand, M. Kuhlen, Piero Madau
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Cylindrical model for the dark matter halo of disk galaxies [PDF]
Brian Slovick
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Modified Newtonian dynamics (MOND) was originally proposed to model galaxy rotation curves without dark matter. However, MOND presents difficulties in explaining the radial acceleration relation observed in galaxy clusters, and moreover, it does not ...
Robert Monjo
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Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients [PDF]
S. Pasetto +4 more
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Spatial Distribution of Intracluster Light versus Dark Matter in Horizon Run 5
One intriguing approach for studying the dynamical evolution of galaxy clusters is to compare the spatial distributions among various components such as dark matter, member galaxies, gas, and intracluster light (ICL).
Jaewon Yoo +13 more
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Polytropic spheres modelling dark matter haloes of dwarf galaxies [PDF]
Jan Novotný +2 more
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