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The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation

Rahmati, Alireza ; Schaye, Joop ; Bower, Richard G. ; Crain, Robert A. ; Furlong, Michelle ; Schaller, Matthieu ; Theuns, Tom

In: Monthly Notices of the Royal Astronomical Society, 2015, vol. 452, no. 2, p. 2034-2056

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    Titre
    • The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation
    Auteur
    • Rahmati, Alireza. Institute for Computational Science, University of Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland
    • Schaye, Joop. Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands
    • Bower, Richard G.. Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
    • Crain, Robert A.. Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands
    • Furlong, Michelle. Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
    • Schaller, Matthieu. Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
    • Theuns, Tom. Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK
    Type de document
    • Postprint
    Langue
    • Anglais
    Publié dans
    • Monthly Notices of the Royal Astronomical Society, 2015, vol. 452, no. 2, p. 2034-2056. Oxford University Press
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:301588
    Summary
    The observed high covering fractions of neutral hydrogen (${\rm H\,\small {\rm I}}$) with column densities above∼1017 cm−2 around Lyman-Break Galaxies (LBGs) and bright quasars at redshifts z∼2-3 has been identified as a challenge for simulations of galaxy formation. We use the Evolution and Assembly of Galaxies and their Environment (EAGLE) cosmological, hydrodynamical simulation, which has been shown to reproduce a wide range of galaxy properties and for which the subgrid feedback was calibrated without considering gas properties, to study the distribution of ${\rm H\,\small {\rm I}}$ around high-redshift galaxies. We predict the covering fractions of strong ${\rm H\,\small {\rm I}}$ absorbers (${N_{\rm H\,\small {I}}}\gtrsim 10^{17} \,{\rm cm^{-2}}$) inside haloes to increase rapidly with redshift but to depend only weakly on halo mass. For massive (M200≳1012M⊙) haloes, the covering fraction profiles are nearly scale-invariant and we provide fitting functions that reproduce the simulation results. While efficient feedback is required to increase the ${\rm H\,\small {\rm I}}$ covering fractions to the high observed values, the distribution of strong absorbers in and around haloes of a fixed mass is insensitive to factor of 2 variations in the strength of the stellar feedback. In contrast, at fixed stellar mass the predicted ${\rm H\,\small {\rm I}}$ distribution is highly sensitive to the feedback efficiency. The fiducial EAGLE simulation reproduces both the observed global column density distribution function of ${\rm H\,\small {\rm I}}$ and the observed radial covering fraction profiles of strong ${\rm H\,\small {\rm I}}$ absorbers around LBGs and bright quasars