Very high energy gamma-ray observations of the galaxy clusters Abell 496 and Abell 85 with HESS

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Table 1:

Properties of the two galaxy clusters. $L_{\rm X, 0.1-2.4}$ is the luminosity in the 0.1-2.4 keV band and $R_{\rm vir}$ is the virial radius.
Cluster	$M_{\rm tot}$ [ $M_{\rm sun}$ ]	$L_{\rm X, 0.1-2.4}$ [erg s^-1]	T [keV]	$R_{\rm vir}$ [Mpc]	Redshift	Distance [Mpc]	Refs.
Abell 496	$3.1\times 10^{14}$	$1.9\times 10^{44}$	4.7	1.4	0.033	134	a, b
Abell 85	$7.6\times 10^{14}$	$4.8\times 10^{44}$	7	1.9	0.055	220	a, c

References: a) Reiprich & Böhringer (2002); b) Markevitch et al. (1999); c) Durret et al. (2005).

Source LaTeX | All tables | In the text

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