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- W2146457805 abstract "Radial velocities and distances of 1136 B-type stars brighter than 10 mag. and lying close to the galactic plane (-10o ≤ b ≤ 10o) are used to de- termine the rotation curve of our Galaxy in the region 7-13 kpc from the ga- lactic center. The derived curve is found to be similar to that obtained from Cepheids Variables and in good agreement with the theoretical curve obtained from dynamical models." @default.
- W2146457805 created "2016-06-24" @default.
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- W2146457805 date "1999-01-01" @default.
- W2146457805 modified "2023-09-27" @default.
- W2146457805 title "Determination of the Galactic Rotation Curve from B-Type Stars" @default.
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