Fundamental Parameters of the Milky Way Galaxy Based on VLBI astrometry
Mareki Honma, Takumi Nagayama, Kazuma Ando, Takeshi Bushimata, Yoon, Kyung Choi, Toshihiro Handa, Tomoya Hirota, Hiroshi Imai, Takaaki Jike, Mi, Kyoung Kim, Osamu Kameya, Noriyuki Kawaguchi, Hideyuki Kobayashi, Tomoharu, Kurayama, Seisuke Kuji, Naoko Matsumoto, Seiji Manabe

TL;DR
This study uses VLBI astrometry of 52 maser sources to precisely determine fundamental parameters of the Milky Way, including the distance to the galactic center, rotation curve shape, and solar motion, with improved accuracy and insights into Galactic structure.
Contribution
It provides new constraints on the Milky Way's fundamental parameters using VLBI data and a Markov chain Monte Carlo analysis, refining previous estimates and revealing correlations among parameters.
Findings
Galactic center distance R_0 = 8.05 +/- 0.45 kpc
Rotation curve is flat between 4 and 13 kpc
Strong correlation between Omega_0 and V_sun
Abstract
We present analyses to determine the fundamental parameters of the Galaxy based on VLBI astrometry of 52 Galactic maser sources obtained with VERA, VLBA and EVN. We model the Galaxy's structure with a set of parameters including the Galaxy center distance R_0, the angular rotation velocity at the LSR Omega_0, mean peculiar motion of the sources with respect to Galactic rotation (U_src, V_src, W_src), rotation-curve shape index, and the V component of the Solar peculiar motions V_sun. Based on a Markov chain Monte Carlo method, we find that the Galaxy center distance is constrained at a 5% level to be R_0 = 8.05 +/- 0.45 kpc, where the error bar includes both statistical and systematic errors. We also find that the two components of the source peculiar motion U_src and W_src are fairly small compared to the Galactic rotation velocity, being U_src = 1.0 +/- 1.5 km/s and W_src = -1.4 +/-…
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