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Table 2:

Cluster properties.
  K. Arnaud$^{\dag }$ Chen et al. (2007)$^{\dag }$ Ikebe et al. (2002)$^{\dag }$ Edge et al. (1992)$^{\dag }$
Cluster kT $\dot{M}$ kT $\dot{M}$ $L_{X}[\rm0.1{-}2.4~keV]$ kT $L_{X}[\rm0.1{-}2.4~keV]$ $L_{X}[\rm 2{-}10~keV]$ $\dot{M}$
  (keV) ( $M_{\odot}~\rm yr^{-1}$) (keV) ( $M_{\odot}~\rm yr^{-1}$) $(\rm h_{70}^{-2}~10^{44}~\rm erg/s)$ (keV) $(h_{70}^{-2}~10^{44}~\rm erg/s)$ $(h_{70}^{-2}~10^{44}~\rm erg/s)$ ( $M_{\odot}~\rm yr^{-1}$)
Abell 85 6.8 128.5 $6.10_{\rm -0.20}^{+0.20}$ $200_{\rm -27}^{+33}$ 13.54 $\pm$ 0.15 $6.51_{\rm -0.23}^{+0.16}$ 1.81 $\pm$ 0.02 10.56 236
Perseus (A426) 6.4 94.9 $6.79_{\rm -0.12}^{+0.12}$ $481_{\rm -32}^{+31}$ - $6.42_{\rm -0.06}^{+0.06}$ 2.93 $\pm$ 0.04 15.40 183
Abell 496 5.7 100.7 $4.13_{\rm -0.08}^{+0.08}$ $114_{\rm -28}^{+35}$ 5.28 $\pm$ 0.07 $4.59_{\rm -0.10}^{+0.10}$ 0.69 $\pm$ 0.01 3.56 112
Abell 3376 - - $4.30_{\rm -0.60}^{+0.60}$ $0_{\rm -0}^{+0}$ 3.02 $\pm$ 0.07 $4.43_{\rm -0.38}^{+0.39}$ 0.74 $\pm$ 0.02 - -
Abell 754 - - $9.00_{\rm -0.50}^{+0.50}$ $0_{\rm -0}^{+0}$ 5.56 $\pm$ 0.15 $9.00_{\rm -0.34}^{+0.35}$ 4.0 $\pm$ 0.10 14.70 24
Hydra A - - $3.80_{\rm -0.20}^{+0.20}$ $293_{\rm -84}^{+50}$ 8.18 $\pm$ 0.06 - - 3.89 315
Centaurus 2.3 31.3 $3.68_{\rm -0.06}^{+0.06}$ $24_{\rm -5}^{+6}$ 1.67 $\pm$ 0.06 - - 0.81 18
Abell 1644 5.1 19.3 $4.70_{\rm -0.70}^{+0.90}$ $0_{\rm -0}^{+0}$ 5.49 $\pm$ 0.48 $4.70_{\rm -0.70}^{+0.90}$ 0.73 $\pm$ 0.06 3.33 19
Abell 1991 4.6 71.0 - - -   - - -
Abell 2052 3.7 30.8 $3.03_{\rm -0.04}^{+0.04}$ $108_{\rm -49}^{+188}$ 3.32 $\pm$ 0.06 $3.12_{\rm -0.09}^{+0.10}$ 0.43 $\pm$ 0.01 1.97 90
Abell 2107 6.5 0.0 - - -   - - -
Ophiuchus - - $10.26_{\rm -0.32}^{+0.32}$ $0_{\rm -0}^{+0}$ - $10.25_{\rm -0.36}^{+0.30}$ 2.2 $\pm$ 0.07 21.28 75
Abell 3667 - - $7_{\rm -0.60}^{+0.60}$ $0_{\rm -0}^{+0}$ 13.27 $\pm$ 0.15 $6.28_{\rm -0.26}^{+0.27}$ 1.78 $\pm$ 0.02 11.59 0
Abell 4059 - - $4.10_{\rm -0.30}^{+0.30}$ $69_{\rm -15}^{+20}$ 3.92 $\pm$ 0.08 $3.94_{\rm -0.15}^{+0.15}$ 0.52 $\pm$ 0.01 2.65 124
Abell 2589 - - $3.70_{\rm -1.10}^{+2.20}$ $19_{\rm -19}^{+53}$ 2.62 $\pm$ 0.06 $3.38_{\rm -0.13}^{+0.13}$ 3.44 $\pm$ 0.08 - -

Notes.  $^{(\dag )}$ All values were converted to a common cosmology with a Hubble constant given as H0=70 km s-1 Mpc-1.


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