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Rotation Curve and Kinematic Propertiesof 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 rotationcurve of the Milky Way spanning the Galactocentric distance intervalfrom 2 to 14 kpc based on observational data for young disk populationsand refine the distance scales of the objects belonging to young diskpopulations (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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