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

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

2009-01-16

arxiv.org/abs/0901.2481v1

Astrophys.J.696:1981-1986,2009

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

The Astrophysical Journal, accepted, 16 pages, 4 Figures

Scientific paper

10.1088/0004-637X/696/2/1981

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 degrees. 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.

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