Cosmological simulations of the circumgalactic medium with 1 kpc resolution: Enhanced HI column densities

Freeke van de Voort*, Volker Springel, Nir Mandelker, Frank C. van den Bosch, Rüdiger Pakmor

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

141 Scopus citations

Abstract

The circumgalactic medium (CGM), i.e. the gaseous haloes around galaxies, is both the reservoir of gas that fuels galaxy growth and the repository of gas expelled by galactic winds. Most cosmological, hydrodynamical simulations focus their computational effort on the galaxies themselves and treat the CGM more coarsely, which means small-scale structure cannot be resolved.We get around this issue by running zoom-in simulations of aMilkyWaymass galaxy with standard mass refinement and additional uniform spatial refinement within the virial radius. This results in a detailed view of its gaseous halo at unprecedented (1 kpc) uniform resolution with only a moderate increase in computational time. The improved spatial resolution does not impact the central galaxy or the average density of the CGM. However, it drastically changes the radial profile of the neutral hydrogen column density,which is enhanced at galactocentric radii larger than 40 kpc. The covering fraction of Lyman-Limit Systems within 150 kpc is almost doubled. We therefore conclude that some of the observational properties of the CGM are strongly resolution dependent. Increasing the resolution in the CGM, without increasing the resolution of the galaxies, is a promising and computationally efficient method to push the boundaries of state-of-the-art simulations.

Original languageAmerican English
Pages (from-to)L85-L89
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume482
Issue number1
DOIs
StatePublished - 1 Jan 2019
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2018 The Author(s).

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: haloes
  • Hydrodynamics
  • Intergalactic medium
  • Methods: numerical

Fingerprint

Dive into the research topics of 'Cosmological simulations of the circumgalactic medium with 1 kpc resolution: Enhanced HI column densities'. Together they form a unique fingerprint.

Cite this