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Galactic & Stellar Dynamics
C. Boily, P. Patsis, S. Portegies Zwart, R. Spurzem and C. Theis (eds)
EAS Publications Series, Vol. 10, 2003
DOI: 10.1051/eas:2003155
Rotation Curve and Kinematic Properties of Young Disk Populations
A.S. Rastorgouev, M.V. Zabolotskikh and A.K. DambisSternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russia
Abstract
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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