S
S. E. de Mink
Researcher at Harvard University
Publications - 232
Citations - 15761
S. E. de Mink is an academic researcher from Harvard University. The author has contributed to research in topics: Stars & Metallicity. The author has an hindex of 60, co-authored 203 publications receiving 13009 citations. Previous affiliations of S. E. de Mink include Max Planck Society & Carnegie Institution for Science.
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Journal ArticleDOI
Binary Interaction Dominates the Evolution of Massive Stars
Hugues Sana,S. E. de Mink,S. E. de Mink,A. de Koter,A. de Koter,Norbert Langer,Chris Evans,Mark Gieles,Eric Gosset,Robert G. Izzard,J.-B. Le Bouquin,Fabian Schneider +11 more
TL;DR: More than 70% of all massive stars will exchange mass with a companion, leading to a binary merger in one-third of the cases, greatly exceed previous estimates and imply that binary interaction dominates the evolution of massive stars, with implications for populations ofmassive stars and their supernovae.
Journal ArticleDOI
Rotating massive main-sequence stars - I. Grids of evolutionary models and isochrones
Ines Brott,Ines Brott,S. E. de Mink,S. E. de Mink,Matteo Cantiello,Norbert Langer,Norbert Langer,A. de Koter,A. de Koter,Chris Evans,Ian Hunter,Carrie Trundle,Jorick S. Vink +12 more
TL;DR: In this paper, a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars is presented to compare with early OB stars in the Small and Large Magellanic Clouds and in the Galaxy.
Journal ArticleDOI
Massive binaries as the source of abundance anomalies in globular clusters
TL;DR: In this paper, the authors compute the evolution of a 20 M star in a close binary considering the effects of non-conservative mass and angular momentum transfer and of rotation and tidal interaction to demonstrate the principle.
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The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population
Hugues Sana,A. de Koter,A. de Koter,S. E. de Mink,S. E. de Mink,P. R. Dunstall,Chris Evans,Vincent Hénault-Brunet,J. Maíz Apellániz,O.H. Ramírez-Agudelo,W. D. Taylor,Nolan R. Walborn,J. S. Clark,Paul A. Crowther,Artemio Herrero,Artemio Herrero,Mark Gieles,Norbert Langer,D. J. Lennon,Jorick S. Vink +19 more
TL;DR: In this paper, the multiplicity properties of the massive O-type star population were analyzed using multi-epoch spectroscopy and variability analysis to identify spectroscopic binaries.
Journal ArticleDOI
The rotation rates of massive stars: the role of binary interaction through tides, mass transfer, and mergers
S. E. de Mink,S. E. de Mink,Norbert Langer,Robert G. Izzard,Hugues Sana,A. de Koter,A. de Koter,A. de Koter +7 more
TL;DR: In this article, it has been shown that 20+5 −10% of all massive main-sequence stars have projected rotational velocities in excess of 200 km s−1.