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The Evolution of The Milky Way pp 125–138Cite as

Wolf-Rayet Stars, Binaries, Black Holes

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 255))

Abstract

We review the literature of the past two decades on the possible evolution from the massive star Wolf-Rayet phase to the black hole phase, and on the masses of WR stars observed in binary systems. A list of 55 WR binaries is presented. The 19 WR binaries with RV solutions have WN star masses in the range 2-55 Moand WC star masses in the range 9-16 Mo. We discuss four candidate WR+BH systems: WR 145a (Cyg X-3), WR 148 (HD 197406), BAT99-102 (R 140a2), and BAT99-116 (Mk 34).

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  1. Space Research Organization Netherlands, Sorbonnelaan 2, Utrecht, NL-3584 CA, the Netherlands

    Karel A. Van der Hucht

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  1. Dipartimento di Astronomia, University of Trieste, Italy

    Francesca Matteucci

  2. Instituto di Astrofisica Spaziale, Fuescoti, Italy

    Franco Giovannelli

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Van der Hucht, K.A. (2000). Wolf-Rayet Stars, Binaries, Black Holes. In: Matteucci, F., Giovannelli, F. (eds) The Evolution of The Milky Way. Astrophysics and Space Science Library, vol 255. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0938-6_13

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