Abstract
About 60% of stars of the disc population in our Galaxy are close binary systems (CBS). Half of the known CBS are spectroscopic binary stars (Kraitcheva et al., 1978).
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© 1982 D. Reidel Publishing Company
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Popova, E.I., Tutukov, A.V., Shustov, B.M., Yungelson, L.R. (1982). On the Distribution of Young Spectroscopic Binary Stars over the Major Semiaxes of their Orbits. In: Kopal, Z., Rahe, J. (eds) Binary and Multiple Stars as Tracers of Stellar Evolution. Astrophysics and Space Science Library, vol 98. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7861-4_17
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DOI: https://doi.org/10.1007/978-94-009-7861-4_17
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