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Table 2

Hydrodynamic scaling relations.

Property Proportionality Scaling  no evoluion of fgas Scaling with empirical evolution

density profile  ∝ ρ   fgas  ∝   ∝ T0.45E(z)1.385
luminositya  ∝   ∝ 
bolom. lum.  ∝   ∝ 
entropy, K  ∝   ∝   ∝ 
gas mass  ∝ ρ   R3   fgas  ∝   ∝ 
YX  ∝ TX   ρ   R3   fgas  ∝   ∝ 
pressure, P(r)  ∝ TX   ρ   fgas  ∝   ∝ 
surf. bright., SX(r)  ∝   ∝   ∝ 

temperature TX  ∝ M2/3E2/3
gas mass fr. fgas  ∝ M0.3E0.3  ∝ M0.3E-0.32
density profile ρ  ∝ M0.3E(z)2.3  ∝ M0.3E1.69
luminositya LX  ∝ M1.6   E2.6   ∝ M1.6   E1.37
bolom. lum. Lbol  ∝ M1.93   E2.93   ∝ M1.93   E2.01
entropy K(r)  ∝ M0.47   E-0.87   ∝ M0.47   E0.98
gas mass Mgas  ∝ M1.3   E0.3   ∝ M1.3   E-0.32
YX TX Mgas  ∝ M1.97   E0.97   ∝ M1.97   E0.35
pressure P(r)  ∝ M0.97   E2.97   ∝ M0.97   E2.35
surf. bright. SX(r)  ∝ M0.93   E3.93   ∝ M0.93   E2.70

Notes. Columns 1 and 2 give the property and its definition (see also Table 1); Col. 3 the scaling relations modified for hydrodynamical effects as described in Sect. 6, based on a redshift-independent fgasTX relation, and Col. 4, redshift dependence implied from the results of Reichert et al. (2011) as given in Eq. (33).

(a)

For temperature independent emissivity (see Table 1 and text).

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