The milky way’s plane of satellites is consistent with λcdm

HIGHLIGHTS

• who: Till Sawala from the Initial conditionsThe simulations used in this work are cosmological zoom-in-constrained simulations, based on initial conditions created for the SIBELIUS project, and designed to reproduce Local Group (LG) analogues within the observed large-scale structure. The simulations assume a u039bCDM cosmology with density parameters u03a90=0., and u03a9u039b=0., for matter and dark energy, respectively, an r.m.s. density variation on a scale of, h, Mpc of u03c38=0., and a Hubble parameter of h=0.6777. We use physical units throughout this work. Building on an octree representation of . . .
  

   

  

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