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WR Stars with Ring Nebulae
Published online by Cambridge University Press: 14 August 2015
Abstract
It is shown that most of usually apparently single nitrogen WR stars with ring emission nebulae around them (WN + Neb) are a probable product of the evolution of a massive close binary with initial masses of components exceeding ∼20 MO.
- Type
- SESSION 6 — LOW MASS WOLF-RAYET STARS RING NEBULAE
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- Copyright
- Copyright © Reidel 1982