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Young W UMa Binaries and the Interaction with their Environment
Published online by Cambridge University Press: 12 April 2016
Extract
It is arpued that late type W UMa binaries undergo mass ejection, mainly through the second Lagragian point, which causes a steady decrease of their mass ratio m2/m1. This makes it reasonable to believe that the W UMa stage is a state of transition between T Tau and normal main sequence stars.
- Type
- Part II: Cataclysmic Variables
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- Copyright
- Copyright © Veröff. Der Remeis-Sterwarte 1977