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- W2149238766 abstract "Abstract A catalogue of open clusters is used to analyze the Galactic kinematics near the Sun. The Galactic open clusters, which are components of Galactic thin disk, were selected for our analysis. Based on kinematical data for around 270 Galactic open clusters, we found the Galactic rotation curve remains flat near the Sun. We also found V e = 6.40±3.39 km s −1 inside the solar circle, which shows a weak trend of stars moving toward the Galactic anti-center." @default.
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- W2149238766 date "2007-10-01" @default.
- W2149238766 modified "2023-09-26" @default.
- W2149238766 title "Galactic kinematics near the sun from open clusters" @default.
- W2149238766 cites W3124275756 @default.
- W2149238766 doi "https://doi.org/10.1017/s1743921308019959" @default.
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