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- W1711646262 abstract "Aims. The detailed structure of the Galactic bulge still remains uncertain. The strong difficulties of obtaining observations of stars in the Galactic bulge have hindered the acquisition of a kinematic representation for the inner kpc of the Milky Way. The observation of the 3-d kinematics in several low foreground extinction windows can solve this problem." @default.
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- W1711646262 date "2012-03-23" @default.
- W1711646262 modified "2023-10-17" @default.
- W1711646262 title "3-dimensional kinematics in low foreground extinction windows of the Galactic bulge" @default.
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- W1711646262 doi "https://doi.org/10.1051/0004-6361/201116522" @default.
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