The distance to a star forming region in the Outer arm of the Galaxy

We performed astrometric observations with the VLBA of WB89−437, an H2O maser source in the Outer spiral arm of the Galaxy. We measure an annual parallax of 0.167±0.006 mas, corresponding to a heliocentric distance of 6.0±0.2 kpc or a Galactocentric distance of 13.4 ± 0.2 kpc. This value for the heliocentric distance is considerably smaller than the kinematic distance of 8.6 kpc. This confirms the presence of a faint Outer arm toward l = 135. We also measured the full space motion of the object and find a large peculiar motion of ∼20 km s toward the Galactic center. This peculiar motion explains the large error in the kinematic distance estimate. We also find that WB89−437 has the same rotation speed as the LSR, providing more evidence for a flat rotation curve and thus the presence of dark matter in the outer Galaxy. Subject headings: astrometry, masers, stars: distances, Galaxy: structure, kinematics and dynamics