تقرير
Evolution of intermediate mass and massive binary stars: physics, mass loss, and rotation
| العنوان: | Evolution of intermediate mass and massive binary stars: physics, mass loss, and rotation |
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| المؤلفون: | Vanbeveren, D., Mennekens, N. |
| سنة النشر: | 2016 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Solar and Stellar Astrophysics |
| الوصف: | 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. Comment: 10 pages, 3 figures, invited paper to appear in the proceedings of the June 2016 conference "The B[e] Phenomenon: Forty Years of Studies" |
| نوع الوثيقة: | Working Paper |
| URL الوصول: | http://arxiv.org/abs/1609.02401 |
| رقم الأكسشن: | edsarx.1609.02401 |
| قاعدة البيانات: | arXiv |
| الوصف غير متاح. |