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We have made VLBI observations at 86 GHz using a 1000-km baseline between Korea and Japan with successful detections of SiO v = 1, J = 2-1 maser emissions from VY CMa and Orion KL in 2001 June. This was the first VLBI result for this baseline and the first astronomical VLBI observation for the Korean telescope. Since then, we observed SiO v = 1, J = 2-1 maser emission in VY CMa in 2002 January and 2003 February and derived the distributions of the maser emissions. Our results show that thedoi:10.1093/pasj/56.3.475 fatcat:5bt7ewusmzcjxb2oxmsdncojku