In the spectra of 139 early-type Large Magellanic Cloud (LMC) stars observed with Far Ultraviolet Spectroscopic Explorer and with deep radio Parkes HI 21cm observations along with those stars, we search for and analyze the absorption and emission from high-velocity gas at +90<={nu}LSR<=+175km/s. The HI column density of the high-velocity clouds (HVCs) along these sightlines ranges from 10^6^M_{sun}_) HVC complex that is linked to stellar feedback occurring in a dwarf spiral galaxy.
Cone search capability for table J/ApJ/702/940/table1 (Summary of the measurements for the high-velocity clouds (HVCs) toward the LMC)