Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-03-08
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
10 pages, 8 figures, to appear in proc. IAU-Symp. 268. C. Charbonnel et al., eds.
Scientific paper
We highlight the role of the light elements (Li, Be, B) in the evolution of massive single and binary stars, which is largely restricted to a diagnostic value, and foremost so for the element boron. However, we show that the boron surface abundance in massive early type stars contains key information about their foregoing evolution which is not obtainable otherwise. In particular, it allows to constrain internal mixing processes and potential previous mass transfer event for binary stars (even if the companion has disappeared). It may also help solving the mystery of the slowly rotating nitrogen-rich massive main sequence stars.
Brott Ines
Cantiello Matteo
de Mink Selma E.
Izzard Robert G.
Langer Norbert
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