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Home All issues Volume 503 / No 1 (August III 2009) A&A, 503 1 (2009) 35-46 Full HTML
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Table 8:

General information for each cluster: the overall (defined here to be from $0{-}2r_{\rm {c}}$) temperature and iron abundance, the overall luminosity, the total number of counts in the cluster, the calculations relevant to the cooling time, and finally the subset as defined in Table 7.
Temperatures and Iron abundances for each full cluster Cooling calculations for each central region Analysis Subset
cluster name $ \it z$ temperature iron abundance # of Counts $\mathcal{L}_{0-2}$ $\mathcal{L}_{0-0.5}$ proton density cooling time age subset #
Abell 1413 $^{\dagger}$ 0.142 $7.0 \pm 0.3 $ $0.46 \pm 0.08$ 11164 5.11 1.95 0.019 3.79 8.55 2
Abell 2204 $^{\dagger}$ 0.152 $4.3 \pm 0.1$ $0.86 \pm 0.08$ 16382 5.17 1.09 0.22 0.24 8.44 1
Abell 665 $^{\dagger}$ 0.182 $8.0 \pm 0.4$ $0.40 \pm 0.08$ 12526 3.89 0.87 0.012 6.91 8.11 2
RX J0439.0+0520 $^{\dagger}$ 0.208 $3.6 \pm 0.2$ $0.76 \pm 0.17$ 2018 1.96 0.75 0.08 0.57 7.83 1
Abell 773 0.217 $8.0 \pm 0.7$ $0.32 \pm 0.13$ 8351 9.24 5.24 0.0058 14.72 7.74 4
Abell 1763 0.223 $7.9 \pm 0.2$ $0.34 \pm 0.04$ 48845 8.81 3.52 0.0062 12.93 7.68 4
Abell 2390 $^{\dagger}$ 0.228 $8.5 \pm 0.2$ $0.43 \pm 0.04$ 36705 10.70 3.41 0.038 1.94 7.63 2
Abell 1835 $^{\dagger}$ 0.253 $6.0 \pm 0.1$ $0.39 \pm 0.01$ 242214 18.20 7.20 0.088 0.71 7.38 1
Abell 697 0.282 ${9.7 \pm 0.7}$ ${0.35 \pm 0.08}$ 13442 16.6 7.75 0.0082 11.15 7.10 4
Abell 611 $^{\dagger}$ 0.288 $7.0 \pm 0.3 $ $0.31 \pm 0.06$ 15213 6.53 2.64 0.019 3.92 7.04 2
MS 1008.1-1224 0.306 $6.3 \pm 0.4$ ${0.35 \pm 0.08}$ 7257 4.18 1.28 0.0082 8.49 6.88 3
MS 2137.3-2353 $^{\dagger}$ 0.313 $4.6 \pm 0.1$ $0.35 \pm 0.04$ 16958 8.29 2.87 0.10 0.60 6.81 1
Abell 1995 0.319 ${8.9 \pm 0.5}$ $0.28 \pm 0.10$ 34062 15.20 5.73 0.0062 13.58 6.73 4
ZWCL 1358+6245 $^{\dagger}$ 0.328 $6.1 \pm 0.3$ $0.39 \pm 0.08$ 8208 3.37 0.94 0.035 1.65 6.68 1
RX J0256.5+0006 0.360 $ 5.0 \pm 0.2$ $0.34 \pm 0.06$ 8608 4.49 1.36 0.0061 11.32 6.40 3
RX J0318.2-0301 0.370 $5.7 \pm 0.3$ $0.28 \pm 0.08$ 7879 3.76 1.31 0.0064 9.16 6.32 3
RX J0426.1+1655 $^{\dagger}$ 0.380 $5.4 \pm 0.4 $ $0.19 \pm 0.07$ 33174 1.55 0.77 0.021 2.83 6.23 1
MACS J2228.5+2036 0.412 $7.1 \pm 0.5$ $0.33 \pm 0.10 $ 6199 15.29 6.24 0.0081 10.30 5.97 8
MACS J2214.9-1359 0.483 $8.8 \pm 0.8 $ $0.29 \pm 0.12$ 3399 14.36 5.20 0.011 7.61 5.43 8
MACS J1311.0-0310${\dagger}$ 0.490 $6.5 \pm 0.6$ $0.45 \pm 0.13$ 2111 10.57 4.60 0.021 3.09 5.38 5
MS 0015.9+1609 0.541 $9.8 \pm 0.6 $ $0.28 \pm 0.06$ 17837 23.57 3.28 0.0041 21.99 5.02 8
MACS 1423.8+2404 $^{\dagger}$ 0.545 $5.3 \pm 0.1 $ $0.54 \pm 0.05$ 17674 10.06 3.31 0.12 0.50 4.99 5
MS 0451.6-0305 0.550 $9.4 \pm 0.7 $ $0.40 \pm 0.11$ 14303 22.11 7.34 0.011 8.32 4.96 8
MACS J2129.4-0741 0.570 $7.0 \pm 1.1 $ $0.41 \pm 0.23$ 1755 10.63 2.59 0.018 4.64 4.82 6
MS 2053.7-0449 0.583 $4.9 \pm 0.5$ $0.28 \pm 0.10$ 1733 1.95 0.41 0.0083 7.75 4.74 7
MACS J0647.7+7015 0.584 $11.5_{\rm -2.0}^{+2.8} $ $0.19_{\rm -0.19}^{+0.26} $ 2717 16.27 7.58 0.013 8.79 4.73 8
RX J1120.1+4318 0.600 $5.2 \pm 0.4$ $0.37 \pm 0.11$ 10239 7.22 3.28 0.0063 11.21 4.63 7
MACS J0744.8+3927${\dagger}$ 0.686 $6.8 \pm 0.7$ $0.51 \pm 0.18$ 1153 9.36 2.66 0.063 1.09 4.11 6
MS 1137.5+6625 0.782 $7.2 \pm 0.6$ $0.26 \pm 0.13$ 4073 6.03 2.07 0.014 5.61 3.59 8
RX J1716.9+6708 0.813 $4.6 \pm 0.5$ $0.57 \pm 0.23$ 1649 6.16 2.21 0.0088 9.69 3.43 7
CL J1226.9+3332 0.890 $11.1 \pm 0.3$ $ 0.20 \pm 0.05$ 29846 20.56 10.06 0.014 7.42 3.07 8
The column $\mathcal{L}_{0-0.5}$ is the luminosity from $0{-}0.5 r_{\rm {c}}$, and $\mathcal{L}_{0-2}$ is the luminosity from $0{-}2r_{\rm {c}}$. The luminosities are in  $\rm erg-s^{-1}$, the times are in Gyr, and the densities are in units of  $\rm cm^{{-3}}$. Galaxy clusters with a dagger (${\dagger}$) next to them have confirmed radio sources likely associated with the cluster. The temperature and iron abundance have the same units as in Table 6.

Source LaTeX | All tables | In the text

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