Comparing galactic satellite properties in hydrodynamical and N-body simulations

Jascha A. Schewtschenko, Andrea Maccio

    Research output: Contribution to journalArticle

    Abstract

    In this work, we examine the different properties of galactic satellites in hydrodynamical and pure dark matter simulations. We use three pairs of simulations (collisional and collisionless) starting from identical initial conditions. We concentrate our analysis on pairs of satellites in the hydro and N-body runs that form from the same Lagrangian region. We look at the radial positions, mass-loss as a function of time and orbital parameters of these 'twin' satellites. We confirm an overall higher radial density of satellites in the hydrodynamical runs, but find that trends in the mass-loss and radial position of these satellites in the inner and outer region of the parent halo differ from the pure dark matter case. In the outskirts of the halo (≈70 per cent of the virial radius), satellites experience a stronger mass-loss and higher dynamical friction in pure dark matter runs. The situation is reversed in the central region of the halo, where hydrodynamical satellites have smaller apocentre distances and suffer higher mass stripping. We partially ascribe this bimodal behaviour to the delayed infall time for hydro satellites, which on average cross the virial radius of the parent halo 0.7Gyr after their dark matter twins. Finally, we briefly discuss the implications of the different set of satellite orbital parameters and mass-loss rates in hydrodynamical simulations within the context of thin-disc heating and destruction.

    Original languageEnglish (US)
    Pages (from-to)878-886
    Number of pages9
    JournalMonthly Notices of the Royal Astronomical Society
    Volume413
    Issue number2
    DOIs
    StatePublished - May 1 2011

    Fingerprint

    simulation
    halos
    dark matter
    orbitals
    radii
    stripping
    destruction
    friction
    heating
    trends
    loss
    parameter

    Keywords

    • Galaxies: haloes
    • Galaxies: structure
    • Gravitation
    • Hydrodynamics
    • Methods: numerical

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Comparing galactic satellite properties in hydrodynamical and N-body simulations. / Schewtschenko, Jascha A.; Maccio, Andrea.

    In: Monthly Notices of the Royal Astronomical Society, Vol. 413, No. 2, 01.05.2011, p. 878-886.

    Research output: Contribution to journalArticle

    Schewtschenko, Jascha A. ; Maccio, Andrea. / Comparing galactic satellite properties in hydrodynamical and N-body simulations. In: Monthly Notices of the Royal Astronomical Society. 2011 ; Vol. 413, No. 2. pp. 878-886.
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