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Rotation Curve and Kinematic Properties of Young Disk Populations

Published online by Cambridge University Press:  22 December 2003

C. Boily ,
P. Patsis ,
S. Portegies ,
R. Spurzem ,
C. Theis ,
A.S. Rastorgouev ,
M.V. Zabolotskikh  and
A.K. Dambis
A.K. Dambis
Affiliation:
Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russia
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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).

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 10: JENAM 2002, Galactic & Stellar Dynamics , 2003 , pp. 223
Copyright
© EAS, EDP Sciences, 2003

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