The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations

Daniel Anglés-Alcázar, Claude André Faucher-Giguère, Dušan Kereš, Philip F. Hopkins, Eliot Quataert, Norman Murray

Research output: Contribution to journalArticle

90 Scopus citations

Abstract

We use cosmological simulations from the FIRE (Feedback In Realistic Environments) project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo mass range Mhalo ~ 1010-1013 M. By tracing cosmic inflows, galactic outflows, gas recycling and merger histories, we quantify the contribution of physically distinct sources of material to galaxy growth. We show that in situ star formation fuelled by fresh accretion dominates the early growth of galaxies of all masses, while the re-accretion of gas previously ejected in galactic winds often dominates the gas supply for a large portion of every galaxy's evolution. Externally processedmaterial contributes increasingly to the growth of central galaxies at lower redshifts. This includes stars formed ex situ and gas delivered by mergers, as well as smooth intergalactic transfer of gas from other galaxies, an important but previously underappreciated growth mode. By z=0, wind transfer, i.e. the exchange of gas between galaxies via winds, can dominate gas accretion on to ~L* galaxies over fresh accretion and standard wind recycling. Galaxies of all masses re-accrete ≳50 per cent of the gas ejected in winds and recurrent recycling is common. The total mass deposited in the intergalactic medium per unit stellar mass formed increases in lower mass galaxies. Re-accretion of wind ejecta occurs over a broad range of time-scales, with median recycling times (~100-350 Myr) shorter than previously found. Wind recycling typically occurs at the scale radius of the halo, independent of halo mass and redshift, suggesting a characteristic recycling zone around galaxies that scales with the size of the inner halo and the galaxy's stellar component.

Original languageEnglish (US)
Pages (from-to)4698-4719
Number of pages22
JournalMonthly Notices of the Royal Astronomical Society
Volume470
Issue number4
DOIs
StatePublished - Oct 2017

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Cosmology: theory
  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: star formation
  • Intergalactic medium

Fingerprint Dive into the research topics of 'The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations'. Together they form a unique fingerprint.

  • Cite this

    Anglés-Alcázar, D., Faucher-Giguère, C. A., Kereš, D., Hopkins, P. F., Quataert, E., & Murray, N. (2017). The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations. Monthly Notices of the Royal Astronomical Society, 470(4), 4698-4719. https://doi.org/10.1093/mnras/stx1517