The effect of gas accretion on the radial gas metallicity profile of simulated galaxies

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  • staa1334

    Final published version, 1.55 MB, PDF document

  • Florencia Collacchioni
  • Claudia D. P. Lagos
  • Peter D. Mitchell
  • Joop Schaye
  • Emily Wisnioski
  • Sofia A. Cora
  • Camila A. Correa

We study the effect of the gas accretion rate ((M) over dot)(accr)) on the radial gas metallicity profile (RMP) of galaxies using the eagle cosmological hydrodynamic simulations, focusing on central galaxies of stellar mass M-* greater than or similar to 10(9) M-circle dot at z

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume495
Issue number3
Pages (from-to)2827-2843
Number of pages17
ISSN0035-8711
DOIs
Publication statusPublished - 23 May 2020

    Research areas

  • methods: numerical, galaxies: evolution, galaxies: formation, STAR-FORMATION RATES, BLACK-HOLE GROWTH, EAGLE SIMULATIONS, SCALING RELATIONS, ABUNDANCE GRADIENTS, COSMOLOGICAL SIMULATIONS, SUPERNOVA FEEDBACK, CHEMICAL EVOLUTION, FORMING GALAXIES, ATOMIC-HYDROGEN

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