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- W2290469564 abstract "Maser stars have been found with radial velocities up to +350 km s-1 and down to −350 km s-1 and exclusively within a few degrees from the Galactic centre. They form two spatially separated streams: one stream is at positive longitudes and consists of stars going away from us and the other is at negative longitudes consisting of stars approaching us. I show that closed orbits in a simple mass model for the bar explain quantitatively the existence of the two streams and the velocities observed. The mass of the bar is estimated on dynamical grounds: 3 × 1010 Msun." @default.
- W2290469564 created "2016-06-24" @default.
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- W2290469564 date "2016-03-01" @default.
- W2290469564 modified "2023-10-18" @default.
- W2290469564 title "Orbits of maser stars in the rotating Galactic bar" @default.
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- W2290469564 doi "https://doi.org/10.1051/0004-6361/201526083" @default.
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