[OI]λ6300 HVC luminosity versus stellar mass (left panel) and mass accretion rate derived from the UV excess (right panel). Gray arrows represent upper limits for [OI]λ6300 line luminosities when no emission in [OI]λ6300 was detected, while light blue arrows represent upper limits for HVC luminosities when only low-velocity [OI]λ6300 emission was detected. Blue filled circles represent blueshifted HVCs, while red filled circles represent redshifted HVCs (systems that did not present a blueshifted component). Luminosities of redshifted HVCs should be considered as lower limits, since the redshifted part of the jet suffers additional extinction from the circumstellar disk.