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Fig. 8


Slopes of the linear fits to 61 “hot” analogs of the mean element abundance ratios, Δ [X/Fe] SUN − STARS, versus the condensation temperature, TC, as a function of the minimum mass of the least massive planet of each planet-host star (left panel), the stellar metallicity (middle panel), and effective temperature (right panel). The mean error bars of the slopes are shown in upper-left corner for planet hosts and upper-right corner for “single” stars. The symbols as in Fig. 7.

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