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Clusters of Galaxies as Self-Gravitating Systems

Florence Durret·Ricardo Demarco·Frederic Magnard·Daniel Gerbal
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Abstract

Self-gravitating systems such as elliptical galaxies appear to have a constant specific entropy and obey a scaling law relating their potential energy to their mass. These properties can be interpreted as due to the physical processes involved in the formation of these structures. Dark matter haloes obtained through numerical simulations have also been found to obey a scaling law relating their potential energy to their mass with the same slope as ellipticals. Since the X-ray gas in clusters is weakly dissipative, we have checked the hypothesis that it might verify similar properties. We have analyzed ROSAT-PSPC images of 24 clusters, and also found that: 1) the Sérsic law parameters (intensity, shape and scale) describing the X-ray gas emission are correlated two by two; 2) the hot gas in all these clusters roughly has the same specific entropy; 3) a scaling law linking the cluster potential energy to the mass of the X-ray gas is observed, with the same slope as for elliptical galaxies and dark matter haloes.

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Florence Durret, Ricardo Demarco, Frederic Magnard, Daniel Gerbal. 2001-05-29. Clusters of Galaxies as Self-Gravitating Systems. https://arxiv.org/abs/astro-ph/0105496

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