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The galactic distribution of 60 young open clusters
Published online by Cambridge University Press: 14 August 2015
Extract
The photometric distances of 60 young galactic clusters (with sp < b3), all observed in UBV or RGU, have been calculated or recalulated according to “method A” (Becker, 1963). The galactic distribution of these clusters, shown in Figure 1, confirms their role of being good spiral tracers.
- Type
- II. THE DISK COMPONENT
- Information
- Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 101 - 104
- Copyright
- Copyright © Reidel 1979