Xu, Y.Y.XuReid, M. J.M. J.ReidMenten, K. M.K. M.MentenZheng, X. W.X. W.ZhengBrunthaler, A.A.BrunthalerMOSCADELLI, LucaLucaMOSCADELLI2022-12-272022-12-2720081743-9213http://hdl.handle.net/20.500.12386/32797We have measured the distance to the high-mass star-forming region G59.7+0.1 (IRAS 19410+2336) and W3OH. Their distances, 2.20 ± 0.11 kpc and 1.95 ± 0.04 kpc, respectively, were determined by triangulation using Very Long Baseline Array (VLBA) observations of 12.2 GHz methanol masers phase-referenced to compact extragalactic radio sources. In addition to the distances, we have also obtained their proper motions.ELETTRONICOenConference paper10.1017/S17439213080191212-s2.0-47049112471https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/distance-to-g59701-and-w3oh/9AE20EDF357A21DD8C2B83AACA5C8189https://api.elsevier.com/content/abstract/scopus_id/470491124712008IAUS..248..214XFIS/05 - ASTRONOMIA E ASTROFISICA