The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
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Final published version, 1.55 MB, PDF document
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 language | English |
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Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 495 |
Issue number | 3 |
Pages (from-to) | 2827-2843 |
Number of pages | 17 |
ISSN | 0035-8711 |
DOIs | |
Publication status | Published - 23 May 2020 |
- 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
Research areas
Links
- https://arxiv.org/pdf/1910.05377.pdf
Submitted manuscript
ID: 247026959