Outer Rotation Curve of the Galaxy with VERA II: Annual Parallax and Proper Motion of the Star-Forming Region IRAS21379+5106
arXiv:1503.07273 · doi:10.1093/pasj/psv012
Abstract
We conducted astrometric VLBI observations of water-vapor maser emission in the massive star forming region IRAS 21379+5106 to measure the annual parallax and proper motion, using VERA. The annual parallax was measured to be mas corresponding to a trigonometric distance of kpc. The proper motion was mas yr. Using this result, the Galactic rotational velocity was estimated to be km s at the Galactocentric distance kpc, when we adopted the Galactic constants kpc and km s. With newly determined distance, {the bolometric luminosity of the central young stellar object was re-evaluated to , which corresponds to spectral type of} B2--B3. Maser features were found to be distributed along a straight line from south-west to north-east. In addition, a vector map of the internal motions constructed from the residual proper motions implies that maser features trace a bipolar flow and that it cannot be explained by simple ballistic motion.
arXiv comment13 pages, 7 figures, 6 tables
References in corpus (3)
- Trigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- Fundamental Parameters of the Milky Way Galaxy Based on VLBI astrometry
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