Baryon content of groups and clusters (Roussel+, 2000)

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Clusters: Galaxy, X-Ray Sources

Scientific paper

Tables 1 and 2 summarize the data taken from the literature (except for A665, whose X-ray parameters were derived by us) used for our study. Tables 3 and 5 present some dynamical quantities for each cluster or group, in the frame of two different normalizations of the scaling law used to compute the virial radius (EMN : Evrard, Metzler & Navarro, 1996ApJ...469..494E ; BN : Bryan & Norman , 1998ApJ...495...80B) Tables 4 and 6 contain average quantities, as a function of temperature category (groups, cool clusters and hot clusters) and at three different density contrasts, again with either EMN or BN normalization. Results emphasize differences arising from the use of two mass estimators, SLM (for scaling law model) and IHE (for isothermal hydrostatic equilibrium). (7 data files).

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