Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation

@article{Shao2018EvolutionOL,
  title={Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation},
  author={Shi Shao and Marius Cautun and Alis J. Deason and Carlos S. Frenk and Tom Theuns},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={479},
  pages={284-296}
}
We investigate the population of dwarf galaxies with stellar masses similar to the Large Magellanic Cloud (LMC) and M33 in the EAGLE galaxy formation simulation. In the field, galaxies reside in haloes with stellar-to-halo mass ratios of 1.03+0.50−0.31×10−2 (68 per cent confidence level); systems like the LMC, which have an SMC-mass satellite, reside in haloes about 1.3 times more massive, which suggests an LMC halo mass at infall, M200=3.4+1.8−1.2×1011M⊙ (68 per cent confidence level… Expand
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