A classical paradox in high-mass star formation is that powerful radiation pressure can halt accretion, preventing further growth of a central star. Disk accretion has been proposed to solve this problem, but the disks and process are poorly understood. We executed high-resolution ($R$=35,000-70,000) iSHELL spectroscopy $K$-band for eleven protostars. Br-$\gamma$ emission was observed toward ei...