Abstract
We analize the general properties of a group of WUMa-type binaries, which show RSCVn-like activity. The position of these stars in the colour-density and mass-orbital momentum diagrams is studied, but no definite answer can be given on the linkage between short period RSCVn systems (SPG) and WUMa systems with RSCVn-like activity (WWG).
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References
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Milano, L.: 1981, in NATO ASI “Photometric and Spectroscopic Binary Systems, E.B. Carling and Z. Kopal (eds.), D. Reidel Publ. Co., Dordrecht, Holland, p. 331.
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Milano, L., Russo, G., Mancuso, S. (1982). On a Possible Linkage between W-Type WUMa Systems and the Short Period RSCVn-Like Binaries. 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_40
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DOI: https://doi.org/10.1007/978-94-009-7861-4_40
Publisher Name: Springer, Dordrecht
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