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On a Possible Linkage between W-Type WUMa Systems and the Short Period RSCVn-Like Binaries

Published online by Cambridge University Press:  12 April 2016

L. Milano ,
G. Russo  and
S. Mancuso
L. Milano
Affiliation:
Capodimonte Astronomical Observatory, Naples, Italy
G. Russo
Affiliation:
Capodimonte Astronomical Observatory, Naples, Italy
S. Mancuso
Affiliation:
Capodimonte Astronomical Observatory, Naples, Italy

Abstract

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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).

Type
Part III: Evolutionary Processes in Close Binary Systems
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 327 - 335
Copyright
Copyright © Reidel 1982

References

Budding, E. et al.: 1982, Astrophys. Space Sci., submitted.Google Scholar
Chaubey, U.S.: 1979, Astrophys. Space Sci., 74, 177.Google Scholar
Hall, D.S.: 1976, Multiple Periodic Variable Stars, IAU Colloquium no. 29 (Budapest), part 1, p. 297, D. Reidel Publ. Co., Dordrecht, Holland.Google Scholar
Milano, L.: 1981, in NATO ASI “Photometric and Spectroscopic Binary Systems, Carling, E.B. and Kopal, Z. (eds.), D. Reidel Publ. Co., Dordrecht, Holland, p. 331.CrossRefGoogle Scholar