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À propos de : The local solar motion and the scalelength of the Galactic disc        

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  • The local solar motion and the scalelength of the Galactic disc
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  • Abstract. It is suggested that the observed variation of velocity dispersion with asymmetric drift is consistent with a local solar motion in the direction of Galactic rotation of ∼11 km s−1, together with a systematic variation of disc scalelength with age.
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