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).

ON A POSSIBLE LI~KAGE BETWEEN W-TYPE WUMa SYSTEMS AND THE SHORT PERIOD RSCVn-LIKE BINARIES

MILANO L.
Membro del Collaboration Group
;
RUSSO G.
Membro del Collaboration Group
;
1982

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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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11588/892630
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