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• W2056579401 abstract "We report on the results of a 14 yr long VLBI study of proper motions in the IC 133 H2O maser source in the galaxy M33. The method of ordered motion parallax was used to model the three-dimensional structure and dynamics of IC 133 and to obtain a distance estimate, 800 ± 180 kpc. Our technique for determining the distance to M33 is independent of calibrations common to other distance indicators, such as Cepheid period-luminosity relations, and therefore provides an important check for previous distance determinations." @default.
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• W2056579401 date "2004-11-10" @default.
• W2056579401 modified "2023-09-27" @default.
• W2056579401 title "The IC 133 Water Vapor Maser in the Galaxy M33: A Geometric Distance" @default.
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• W2056579401 doi "https://doi.org/10.1086/424731" @default.
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