J
Jorick S. Vink
Researcher at Armagh Observatory
Publications - 338
Citations - 21058
Jorick S. Vink is an academic researcher from Armagh Observatory. The author has contributed to research in topics: Stars & Stellar evolution. The author has an hindex of 70, co-authored 311 publications receiving 18826 citations. Previous affiliations of Jorick S. Vink include University of California, Santa Barbara & Goddard Space Flight Center.
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Mass-loss predictions for O and B stars as a function of metallicity
TL;DR: In this paper, a grid of massive star wind models and mass-loss rates for a wide range of metal abundances between 1=100 Z=Z 10 was calculated and the mass loss rate was shown to be constant in the range between 1/30 Z =Z 3.
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Mass-loss predictions for O and B stars as a function of metallicity
TL;DR: In this paper, a grid of massive star wind models and mass-loss rates for a wide range of metal abundances between 1/100 and 10 Z/Zsun was calculated.
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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.
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Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
Ines Brott,Selma E. de Mink,Matteo Cantiello,Norbert Langer,Alex de Koter,Chris Evans,Ian Hunter,Carrie Trundle,Jorick S. Vink +8 more
TL;DR: In this article, 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.
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On the maximum mass of stellar black holes
Krzysztof Belczynski,Krzysztof Belczynski,Tomasz Bulik,Chris L. Fryer,Chris L. Fryer,Ashley J. Ruiter,Ashley J. Ruiter,Francesca Valsecchi,Jorick S. Vink,Jarrod R. Hurley +9 more
TL;DR: In this paper, the authors present the spectrum of compact object masses: neutron stars and black holes (BHs) that originate from single stars in different environments and calculate the dependence of maximum BH mass on metallicity and on some specific wind mass loss rates.