Table 2: The radius at the center of the last radial bin considered in the gas density fits and the best-fit parameters from fitting Eq. (3) to the data ($1\sigma $ errors in parenthesis).
Cluster $R_{{\rm\rho,max}}$ $\rho_0$ $r_{{\rm c}}$ $\beta$
  (kpc) ( $10^{-20}~{\rm g}/{\rm m}^3$) (kpc)  
NGC 533 160 1.85(0.77) 7(2) 0.46(0.01)
Virgo 35 8.14(0.85) 3(1) 0.33(0.01)
A262 199 4.54(0.91) 5(1) 0.33(0.01)
Sérsic 159-3 499 4.36(0.06) 35(1) 0.59(0.01)
MKW 9 238 67.7(16.29) 19(8) 0.32(0.02)
2A 0335+096 309 8.24(0.49) 20(2) 0.53(0.01)
MKW 3s 402 2.61(0.12) 35(2) 0.49(0.01)
A2052 319 4.02(0.36) 19(2) 0.45(0.02)
A4059 412 1.71(0.18) 48(7) 0.50(0.02)
Hydra A 673 5.13(0.70) 29(5) 0.52(0.02)
A496 193 5.14(0.14) 16(1) 0.42(0.01)
A3112 645 4.15(0.35) 41(4) 0.55(0.02)
A1795 553 4.26(0.18) 42(3) 0.52(0.01)
A399 606 0.72(0.08) 76(15) 0.38(0.03)
Perseus 229 7.27(0.52) 28(3) 0.53(0.02)
A1835 831 5.24(0.23) 80(5) 0.62(0.02)

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