3D views of T CrB in quiescence from the radiative modeling carried out in Sect. 7, for the RG filling completely its Roche lobe, the disk extending to the standard outer radius of twice its circularization value, an orbital inclination of 61$\stackrel{°}{.}$5, and masses of the WD and the RG of 1.35 and 0.93 M_⊙, respectively (cf. Table 4). The stretching of the black-to-white color palette is different for the RG and for the disk + hot spot, respectively 3450–3600 K and 1400–1900 K.