Fig. 7.
Spectral energy distribution (SED) of the primary HIP 79124 A0V star. Top panel: a BT-Settl model (Allard et al. 2012) of Teff = 9200 K and log g = 4.5 dex is fitted to the flux values at ≤10 μm compiled from the literature (see Table 4). Bottom panel: G-value (Cushing et al. 2008) for BT-Settl models with different Teff. The orange dashed line shows the upper limit for the considered well-fitting models.
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