Abstract
A relation between the age of 40 visual binaries and their space-motion components has been derived. It appears that in the U, V plane the distribution of the young stars is at right angle to that of the old and very old stars.
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References
Bakos, G. A.: Thesis, University of Toronto (1959).
Bakos, G. A.: J. Roy. Astron, Soc. Can. 65, 222 (1971).
Doucet, C: Thesis, University of Waterloo (1971).
Eggen, O. J.: Astron. J. 68, 483 (1963).
Astrophys. J. 126, 509 (1957).
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© 1974 Springer-Verlag, Berlin, Heidelberg
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Bakos, G.A. (1974). Kinematic Properties of Selected Visual Binaries. In: Mavridis, L.N. (eds) Proceedings of the First European Astronomical Meeting Athens, September 4–9, 1972. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-65666-8_8
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DOI: https://doi.org/10.1007/978-3-642-65666-8_8
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