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arXiv · 1609.02401

Evolution of intermediate mass and massive binary stars: physics, mass loss, and rotation

D. Vanbeveren·N. Mennekens
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Abstract

In the present review we discuss the past and present status of the interacting OB-type binary frequency. We critically examine the popular idea that Be-stars and supergiant sgB[e] stars are binary evolutionary products. The effects of rotation on stellar evolution in general, stellar population studies in particular, and the link with binaries will be evaluated. Finally a discussion is presented of massive double compact star binary mergers as possible major sites of chemical enrichment of r-process elements and as the origin of recent aLIGO GW events.

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D. Vanbeveren, N. Mennekens. 2016-09-08. Evolution of intermediate mass and massive binary stars: physics, mass loss, and rotation. https://arxiv.org/abs/1609.02401

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