Position of HD 85567 (red square) in the size–luminosity diagram of T Tauri stars, Herbig Ae, and Herbig Be stars. The data are taken from the literature (Eisner et al. 2004; Monnier et al. 2005; Kraus et al. 2008a; Pinte et al. 2008; Weigelt et al. 2011; Chen et al. 2012; Kreplin et al. 2012; Vural et al. 2012; Wang et al. 2012; Kreplin et al. 2013; Vural et al. 2014). The solid line shows the theoretical dependence of the inner ring radius on the luminosity for an optically thin disk hole and a dust sublimation temperature of 1500 K (Monnier et al. 2005).