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Astronomy Reports

, Volume 63, Issue 4, pp 249–262 | Cite as

On the Inner Structure of Virialized Clusters

  • A. Del PopoloEmail author
  • Xiguo Lee
Article
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Abstract

In the present paper, we studied the correlations among different quantities in the clusters of galaxies observed by Newman et al. We found an anti-correlation among the slope α, the effective radius, Re, and a correlation among the core radius rcore and Re. Moreover, the mass in 100 kpc (mainly dark matter) is correlated with the mass inside 5 kpc (mainly baryons). The previous correlations can be understood in a two phase formation model: a first dissipative phase forming the proto-BCG and a second dissipationless phase, in which the inner density profile is flattened by the interaction of baryonic clumps and the DMhalo through dynamical friction (DF).

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© Pleiades Publishing, Ltd. 2019

Authors and Affiliations

  1. 1.Dipartimento di Fisica e AstronomiaUniversità di CataniaCataniaItaly
  2. 2.Institute of Modern PhysicsChinese Academy of SciencesBeijingPeople’s Republic of China
  3. 3.INFN Sezione di CataniaCataniaItaly

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