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...
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Published in | Astronomy letters Vol. 28; no. 7; pp. 454 - 464 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Heidelberg
Springer Nature B.V
01.07.2002
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Subjects | |
Online Access | Get full text |
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