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.
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Tutukov, A. (1982). WR Stars with Ring Nebulae. In: De Loore, C.W.H., Willis, A.J. (eds) Wolf-Rayet Stars: Observations, Physics, Evolution. International Astronomical Union/Union Astronomique Internationale, vol 99. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7910-9_65
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DOI: https://doi.org/10.1007/978-94-009-7910-9_65
Publisher Name: Springer, Dordrecht
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