EAS Publications Series
Volume 10, 2003JENAM 2002, Galactic & Stellar Dynamics
|Page(s)||223 - 223|
|Published online||22 December 2003|
C. Boily, P. Patsis, S. Portegies Zwart, R. Spurzem and C. Theis (eds)
EAS Publications Series, 10 (2003) 223
Rotation Curve and Kinematic Properties of Young Disk Populations
Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russia
We use the method of statistical parallaxes to construct the rotation curve of the Milky Way spanning the Galactocentric distance interval from 2 to 14 kpc based on observational data for young disk populations and refine the distance scales of the objects belonging to young disk populations (classical Cepheids, young open clusters, blue supergiants, HII regions, and HI).
© EAS, EDP Sciences, 2003
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