The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores Journal Articles uri icon

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abstract

  • We use 31 simulated galaxies from the MaGICC project to investigate the effects of baryonic feedback on the density profiles of dark matter (DM) haloes. The sample covers a wide mass range: 9.4e9

authors

  • Di Cintio, Arianna
  • Brook, Chris B
  • Macciò, Andrea V
  • Stinson, Greg S
  • Knebe, Alexander
  • Dutton, Aaron A
  • Wadsley, James

publication date

  • January 1, 2014