Kinematic parameters of young subsystems and the galactic rotation curve

We analyze the space velocities of blue supergiants, long-period Cepheids, and young open star clusters (OSCs), as well as the H I and H II radial-velocity fields by the maximum-likelihood method. The distance scales of the objects are matched both by comparing the first derivatives of the angular v...

Full description

Saved in:
Bibliographic Details
Published inAstronomy letters Vol. 28; no. 7; pp. 454 - 464
Main Authors Zabolotskikh, M V, Rastorguev, A S, Dambis, A K
Format Journal Article
LanguageEnglish
Published Heidelberg Springer Nature B.V 01.07.2002
Subjects
Online AccessGet full text

Cover

Loading…