C
Chen Wang
Researcher at University of Bonn
Publications - 15
Citations - 352
Chen Wang is an academic researcher from University of Bonn. The author has contributed to research in topics: Stars & Stellar evolution. The author has an hindex of 5, co-authored 15 publications receiving 136 citations.
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Journal ArticleDOI
Properties of OB star-black hole systems derived from detailed binary evolution models
Norbert Langer,Norbert Langer,C. Schürmann,C. Schürmann,K. Stoll,Pablo Marchant,Pablo Marchant,D. J. Lennon,D. J. Lennon,Laurent Mahy,S. E. de Mink,S. E. de Mink,M. Quast,W. Riedel,Hugues Sana,Peter Schneider,A. Schootemeijer,Chen Wang,Leonardo A. Almeida,Joachim M. Bestenlehner,J. Bodensteiner,Norberto Castro,Simon Clark,Paul A. Crowther,Philip Dufton,Chris Evans,Luca Fossati,Götz Gräfener,L. Grassitelli,N. J. Grin,Ben Hastings,A. Herrero,A. de Koter,A. de Koter,Athira Menon,Lee Patrick,Joachim Puls,Mathieu Renzo,Mathieu Renzo,Andreas Sander,Fabian Schneider,Fabian Schneider,K. Sen,K. Sen,Tomer Shenar,S. Simón-Días,Thomas M. Tauris,Frank Tramper,Jorick S. Vink,X. T. Xu +49 more
TL;DR: In this article, the authors analyzed a large grid of detailed binary evolution models at LMC metallicity with initial primary masses between 10 and 40 M, and identified the model systems that potentially evolve into a binary consisting of a black hole and a massive main-sequence star.
Journal ArticleDOI
Constraining mixing in massive stars in the Small Magellanic Cloud
TL;DR: In this paper, the authors investigate models for massive stars in the Small Magellanic Cloud (SMC), for which stellar-wind mass loss is less important than for their metal-rich counterparts.
Journal ArticleDOI
Effects of Close Binary Evolution on the Main-sequence Morphology of Young Star Clusters
Chen Wang,Norbert Langer,A. Schootemeijer,Norberto Castro,Sylvia Adscheid,Pablo Marchant,Ben Hastings +6 more
TL;DR: In this paper, the authors used a dense model grid of more than 50,000 detailed binary-evolution calculations to show several distinct, coeval main-sequence (MS) components, most notably an extended MS turnoff region, and a group of nearcritical rotating stars that is spread over a large luminosity range on the red side of the classical MS.
Journal ArticleDOI
Properties of OB star-black hole systems derived from detailed binary evolution models
Norbert Langer,Norbert Langer,C. Schürmann,C. Schürmann,K. Stoll,Pablo Marchant,Pablo Marchant,D. J. Lennon,D. J. Lennon,Laurent Mahy,S. E. de Mink,S. E. de Mink,M. Quast,W. Riedel,Hugues Sana,Peter Schneider,A. Schootemeijer,Chen Wang,Leonardo A. Almeida,Joachim M. Bestenlehner,J. Bodensteiner,Norberto Castro,Simon Clark,Paul A. Crowther,Philip Dufton,Chris Evans,Luca Fossati,Götz Gräfener,L. Grassitelli,N. J. Grin,Ben Hastings,A. Herrero,A. de Koter,A. de Koter,Athira Menon,Lee Patrick,Joachim Puls,Mathieu Renzo,Mathieu Renzo,Andreas Sander,Fabian Schneider,Fabian Schneider,K. Sen,K. Sen,Tomer Shenar,S. Simón-Días,Thomas M. Tauris,Frank Tramper,Jorick S. Vink,X. T. Xu +49 more
TL;DR: In this paper, the authors analyzed a large grid of detailed binary evolution models at LMC metallicity with initial primary masses between 10 and 40 Msun, and identified which model systems potentially evolve into a binary consisting of a black hole and a massive main sequence star.
Journal ArticleDOI
The single star path to Be stars
TL;DR: In this article, the authors identify the main effects which are responsible for single stars to approach critical rotation as functions of initial mass and metallicity, and predict the properties of populations of rotating single stars.