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Showing 1–3 of 3 results
Advanced filters: Author: Mark Vogelsberger Clear advanced filters

  • JWST has revealed many prolate, filamentary galaxies at z ≈ 3–8. Hydrodynamical simulations reproduce this trend only in warm or wave dark matter models, where smooth filamentary accretion dominates over the hierarchical fragmentation seen with cold dark matter.

    • Alvaro Pozo
    • Tom Broadhurst
    • Rogier Windhorst
    Research
    Nature Astronomy
    P: 1-11

  • Cosmological hydrodynamical simulations of the ΛCDM Universe show that isolated quenched ultra-diffuse galaxies are formed as backsplash galaxies that were once satellites of another galactic group or cluster halo but are today a few megaparsecs away from them.

    • José A. Benavides
    • Laura V. Sales
    • Lars Hernquist
    Research
    Nature Astronomy
    Volume: 5, P: 1255-1260

  • Cosmological computer simulations of galaxy formation emerged as the primary tool to study structure formation in the Universe. This Technical Review describes the main techniques and ingredients of such simulations and their application to develop and constrain galaxy formation theories.

    • Mark Vogelsberger
    • Federico Marinacci
    • Ewald Puchwein
    Reviews
    Nature Reviews Physics
    Volume: 2, P: 42-66