An interferometric study of the post-AGB binary 89 Herculis - II. Radiative transfer models of the circumbinary disk

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Fig. 7

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NPOI and VEGA squared visibilities at 673 nm. Our complete grid of double-power-law MCMax models is also displayed (see Sect. 5). The best-fit models listed in Table 1 are shown with the same color coding as in Figs. 1–5.

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