1. The Bar and Spiral Structure Legacy (BeSSeL) Survey: Mapping the Milky Way with VLBI Astrometry
- Author
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K. M. Menten, B. Zhang, Mark J. Reid, Thomas M. Dame, Xingwu Zheng, Yuanwei Wu, Y. K. Choi, G. A. Moellenbrock, Luca Moscadelli, Mayumi Sato, K. L. J. Rygl, Ye Xu, Andreas Brunthaler, K. Hachisuka, Alberto Sanna, K. Immer, and Anna Bartkiewicz
- Subjects
Proper motion ,Milky Way ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,01 natural sciences ,law.invention ,law ,0103 physical sciences ,Very-long-baseline interferometry ,Astrophysics::Solar and Stellar Astrophysics ,Maser ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Spiral ,Physics ,010308 nuclear & particles physics ,Galactic Center ,Astronomy ,Astronomy and Astrophysics ,Astrometry ,Astrophysics - Astrophysics of Galaxies ,Galaxy ,Space and Planetary Science ,13. Climate action ,Astrophysics of Galaxies (astro-ph.GA) ,Astrophysics::Earth and Planetary Astrophysics - Abstract
Astrometric Very Long Baseline Interferometry (VLBI) observations of maser sources in the Milky Way are used to map the spiral structure of our Galaxy and to determine fundamental parameters such as the rotation velocity ($\Theta_0$) and curve and the distance to the Galactic center (R$_0$). Here, we present an update on our first results, implementing a recent change in the knowledge about the Solar motion. It seems unavoidable that the IAU recommended values for R$_0$ and $\Theta_0$ need a substantial revision. In particular the combination of 8.5 kpc and 220 \kms\, can be ruled out with high confidence. Combining the maser data with the distance to the Galactic center from stellar orbits and the proper motion of Sgr\,A* gives best values of R$_0$ = 8.3 $\pm$ 0.23 kpc and $\Theta_0$ = 239 or 246 $\pm$ 7 \kms, for Solar motions of V$_ \odot$ = 12.23 and 5.25 \kms, respectively. Finally, we give an outlook to future observations in the Bar and Spiral Structure Legacy (BeSSeL) Survey., Comment: 6 pages, 3 figures. 'Highlight talk' held at the Meeting of the Astronomische Gesellschaft (2010). To be published in Reviews in Modern Astronomy, Volume 23
- Published
- 2011