Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback

Taysun Kimm, Renyue Cen, Julien Devriendt, Yohan Dubois, Adrianne Slyz

Research output: Contribution to journalArticle

48 Citations (Scopus)

Abstract

To better understand the impact of supernova (SN) explosions on the evolution of galaxies, we perform a suite of high-resolution (12 pc), zoom-in cosmological simulations of a Milky Way-like galaxy at z = 3 with adaptive mesh refinement. We find that SN explosions can efficiently regulate star formation, leading to the stellar mass and metallicity consistent with the observed mass-metallicity relation and stellar mass-halo mass relation at z ~ 3. This is achieved by making three important changes to the classical feedback scheme: (i) the different phases of SN blast waves are modelled directly by injecting radial momentum expected at each stage, (ii) the realistic time delay of SNe is required to disperse very dense gas before a runaway collapse sets in, and (iii) a non-uniform density distribution of the interstellarmedium (ISM) is taken into account below the computational grid scale for the cell in which an SN explodes. The simulated galaxy with the SN feedback model shows strong outflows, which carry approximately 10 times larger mass than star formation rate, as well as smoothly rising circular velocity. Although the metallicity of the outflow depends sensitively on the feedback model used, we find that the accretion rate and metallicity of the cold flow around the virial radius is impervious to SN feedback. Our results suggest that understanding the structure of the turbulent ISM may be crucial to assess the role of SN and other feedback processes in galaxy formation theory.

Original languageEnglish
Pages (from-to)2900-2921
Number of pages22
JournalMonthly Notices of the Royal Astronomical Society
Volume451
Issue number3
DOIs
Publication statusPublished - 2015 Jan 1

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supernovae
star formation
galaxies
metallicity
explosion
outflow
stellar mass
explosions
Milky Way Galaxy
computational grids
momentum
galactic evolution
blasts
star formation rate
accretion
density distribution
halos
time lag
gas
simulation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Kimm, Taysun ; Cen, Renyue ; Devriendt, Julien ; Dubois, Yohan ; Slyz, Adrianne. / Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 451, No. 3. pp. 2900-2921.
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Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback. / Kimm, Taysun; Cen, Renyue; Devriendt, Julien; Dubois, Yohan; Slyz, Adrianne.

In: Monthly Notices of the Royal Astronomical Society, Vol. 451, No. 3, 01.01.2015, p. 2900-2921.

Research output: Contribution to journalArticle

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