The Geometric Distance and Proper Motion of the Triangulum Galaxy (M33)

  title={The Geometric Distance and Proper Motion of the Triangulum Galaxy (M33)},
  author={Andreas Brunthaler and Mark J. Reid and Heino Falcke and Lincoln J. Greenhill and Christian Henkel},
  pages={1440 - 1443}
We measured the angular rotation and proper motion of the Triangulum Galaxy (M33) with the Very Long Baseline Array by observing two H2O masers on opposite sides of the galaxy. By comparing the angular rotation rate with the inclination and rotation speed, we obtained a distance of 730 ± 168 kiloparsecs. This distance is consistent with the most recent Cepheid distance measurement. M33 is moving with a velocity of 190 ± 59 kilometers per second relative to the Milky Way. These measurements… 

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