High-resolution near-ultraviolet spectra of the yellow hypergiants HR 8752 and rho Cassiopeiae indicate high effective temperatures, placing both stars near the low-T_eff border of the ``yellow evolutionary void.'' At present, the temperature of HR 8752 is higher than ever. For this star we found T_eff=7900+/-200 K, whereas rho Cassiopeiae has T_eff=7300+/-200 K. Both HR 8752 and rho Cassiopeiae have developed strong stellar winds with V_∞~=120 and V_∞~=100 km s^-1, respectively. For HR 8752 we estimate an upper limit for the spherically symmetric mass loss of 6.7x10^-6 M_solar yr^-1. Over the past decades two yellow hypergiants appear to have approached an evolutionary phase, which has never been observed before. We present the first spectroscopic evidence of the blueward motion of a cool super/hypergiant on the H-R diagram.