Shock waves in and around clusters of galaxies

  • Hong, Sung-Wook E. (Department of Astronomy and Space Science, Chungnam National University) ;
  • Ryu, Dong-Su (Department of Astronomy and Space Science, Chungnam National University) ;
  • Kang, Hye-Sung (Department of Earth Sciences, Pusan National University)
  • Published : 2012.04.03

Abstract

We examine the distribution and properties of shock waves within a couple of Mpc from cluster center with single-level grid simulations using up to 20483 grid zones. The effects of cooling/heating and feedbacks from galaxies are also incorporated. There are two different populations of shocks, merger shocks and accretion shocks. We discuss the manifestation of shocks through radio relics.

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