Cosmological simulations of the intracluster medium
(2004)
Journal Article
Kay, S. T., Thomas, P. A., Jenkins, A., & Pearce, F. R. (2004). Cosmological simulations of the intracluster medium. Monthly Notices of the Royal Astronomical Society, 355, 1091-1104. https://doi.org/10.1111/j.1365-2966.2004.08383.x
Outputs (6)
The subhalo populations of ΛCDM dark haloes (2004)
Journal Article
Gao, L., White, S., Jenkins, A., Stoehr, F., & Springel, V. (2004). The subhalo populations of ΛCDM dark haloes. Monthly Notices of the Royal Astronomical Society, 355, 819-834. https://doi.org/10.1111/j.1365-2966.2004.08360.x
The inner structure of ΛCDM haloes - II. Halo mass profiles and low surface brightness galaxy rotation curves (2004)
Journal Article
Hayashi, E., Navarro, J., Power, C., Jenkins, A., Frenk, C., White, S., …Quinn, T. (2004). The inner structure of ΛCDM haloes - II. Halo mass profiles and low surface brightness galaxy rotation curves. Monthly Notices of the Royal Astronomical Society, 355, 794-812. https://doi.org/10.1111/j.1365-2966.2004.08359.x
Galaxies and subhaloes in ΛCDM galaxy clusters (2004)
Journal Article
Gao, L., De Lucia, G., White, S., & Jenkins, A. (2004). Galaxies and subhaloes in ΛCDM galaxy clusters. Monthly Notices of the Royal Astronomical Society, 352, L1-L5. https://doi.org/10.1111/j.1365-2966.2004.08098.x
Early Formation and Late Merging of the Giant Galaxies (2004)
Journal Article
Gao, L., Loeb, A., Peebles, P., White, S. D., & Jenkins, A. (2004). Early Formation and Late Merging of the Giant Galaxies. Astrophysical Journal, 614, 17-25. https://doi.org/10.1086/423444
The inner structure of ACDM haloes - III. Universality and asymptotic slopes (2004)
Journal Article
Navarro, J., Hayashi, E., Power, C., Jenkins, A., Frenk, C., White, S., …Quinn, T. (2004). The inner structure of ACDM haloes - III. Universality and asymptotic slopes. Monthly Notices of the Royal Astronomical Society, 349(3), 1039-1051. https://doi.org/10.1111/j.1365-2966.2004.07586.xWe investigate the mass profile of cold dark matter (ΛCDM) haloes using a suite of numerical simulations spanning five decades in halo mass, from dwarf galaxies to rich galaxy clusters. These haloes typically have a few million particles within the v... Read More about The inner structure of ACDM haloes - III. Universality and asymptotic slopes.