Abstract
W75N is a star-forming region containing ultracompact H II regions as well as OH, H2O, and methanol masers. The VLBA maps obtained show that the masers are located in a thin disk rotating around an O star, which is the exciting star for the ultracompact H II region VLA1. A separate group of maser spots is associated with the ultracompact H II region VLA2. The radial velocity of the maser spots varies across the disk from 3.7 to 10.9 km/s. The disk diameter is 4000 AU. The maser spots revolve in Keplerian orbits around the O9 star.
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 78, No. 12, 2001, pp. 1073–1080.
Original Russian Text Copyright © 2001 by Slysh, Val’tts, Migenes.
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Slysh, V.I., Val’tts, I.E. & Migenes, V. A magnetized disk around an O star in W75N. A VLBI map of the OH maser. Astron. Rep. 45, 942–948 (2001). https://doi.org/10.1134/1.1426124
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DOI: https://doi.org/10.1134/1.1426124