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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2722
Abstract: The galaxy luminosity function and galaxy stellar mass function are fundamental statistics to test the galaxy formation models. Theoretical predictions based on cosmological simulations can deviate from observations, especially at bright and faint ends. In…
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Keywords:
galaxy;
mass;
cosmological simulations;
function ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab496
Abstract: The past decade has seen significant progress in understanding galaxy formation and evolution using large-scale cosmological simulations. While these simulations produce galaxies in overall good agreement with observations, they employ different sub-grid models for galaxies…
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Keywords:
mbh relation;
mass;
mass function;
relation ... See more keywords
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Published in 2022 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad998
Abstract: Wave (fuzzy) dark matter ($\psi \rm {DM}$) consists of ultralight bosons, featuring a solitonic core within a granular halo. Here we extend $\psi \rm {DM}$ to two components, with distinct particle masses m and coupled…
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Keywords:
soliton;
component;
cosmological simulations;
minor component ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stw2957
Abstract: Recent studies have revealed an oscillating asymmetry in the vertical structure of the Milky Way's disc. Here we analyze 16 high-resolution, fully cosmological simulations of the evolution of individual Milky Way-sized galaxies, carried out with…
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Keywords:
warps waves;
waves stellar;
milky way;
cosmological simulations ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx2319
Abstract: We introduce the Lomonosov suite of high-resolution N-body cosmological simulations covering a full box of size 32 h(-1) Mpc with low-mass resolution particles (2 x 10(7) h(-1) M-circle dot) and th ...
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Keywords:
pushing low;
halo concentration;
cosmological simulations;
low mass ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx2787
Abstract: The formation and evolution of gravitationally bound, star forming substructures in tidal tails of interacting galaxies, called tidal dwarf galaxies (TDG), has been studied, until now, only in idealized simulations of individual pairs of interacting…
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Keywords:
tdg candidates;
galaxies cosmological;
cosmological simulations;
tidal dwarf ... See more keywords
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Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty610
Abstract: The metallicity of strong HI systems, spanning from damped Lyman-alpha absorbers (DLAs) to Lyman-limit systems (LLSs) is explored between z = 5->0 using the EAGLE high-resolution cosmological hydrodynamic simulation of galaxy formation. The metallicities of…
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Keywords:
eagle cosmological;
metallicity distribution;
distribution systems;
cosmological simulations ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz2076
Abstract: We study influence by models of interstellar medium (ISM) on properties of galaxies in cosmological simulations. We examine three models widely used in previous studies. The ISM models impose different equations of state on dense…
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Keywords:
ism;
formation;
galaxies cosmological;
cosmological simulations ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society: Letters"
DOI: 10.1093/mnrasl/sly190
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…
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Keywords:
resolution;
column;
circumgalactic medium;
cosmological simulations ... See more keywords