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- W124539562 abstract "We are studying the kinematic structure of our Galaxy by detecting SiO maser lines around 43 GHz with the Nobeyama 45-m telescope. Till today, about 500 IRAS sources (AGB stars) in the central region of the Galaxy are observed and the radial velocities of about 300 detected sources are obtained. The longitude-velocity map of SiO sources clearly shows a presence of forbidden regions (holes) which are located at the same positions of HI and CO holes. The presence of holes is interpreted as a streaming motions of stars due to a bar structure of the Galactic bulge" @default.
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- W124539562 date "1998-01-01" @default.
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- W124539562 title "1.5. SiO maser sources in the Galactic bulge and a kinematic signature of the bar structure" @default.
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- W124539562 doi "https://doi.org/10.1017/s0074180900083844" @default.
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