J. S. Vink

Physics and Astronomy · Physical Sciences

74h-index18.8kcitations529works3.92yr avg
OpenAlex↗ORCID↗Google Scholar↗

Accepting Students?

No reports yet. Know if this professor is taking students?

Research Topics

Stellar, planetary, and galactic studies(413), Astronomy and Astrophysical Research(256), Astrophysics and Star Formation Studies(246), Gamma-ray bursts and supernovae(162), Astronomical Observations and Instrumentation(75)

Publications521 total

Little Red Dots as Globular Clusters in Formation
arXiv (Cornell University)·2026Open Access
Little Red Dots as Globular Clusters in Formation
ArXiv.org·2026Open Access
Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
Astronomy and Astrophysics·2026Open Access
Hydrodynamical mass-loss rates for very massive stars
Springer Link (Chiba Institute of Technology)·2026
Hydrodynamical mass-loss rates for Very Massive Stars. I. Investigating the wind kink
arXiv (Cornell University)·2025Open Access
Discovery of a transitional type of evolved massive star with a hard ionizing flux
Nature Astronomy·2025· 1 cited
Black Holes at high and low metallicity
arXiv (Cornell University)·2025Open Access
Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
Astronomy and Astrophysics·2025Open Access
Minimum and maximum mass-luminosity relations for stripped stars
Astronomy and Astrophysics·2025Open Access
A high fraction of close massive binary stars at low metallicity
Nature Astronomy·2025· 8 citedOpen Access
Minimum and maximum mass-luminosity relations for stripped stars
arXiv (Cornell University)·2025Open Access
Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies
Monthly Notices of the Royal Astronomical Society·2025· 4 citedOpen Access
X-Shooting ULLYSES: Massive stars at low metallicity
Astronomy and Astrophysics·2025· 2 citedOpen Access
Near-Eddington mass loss of hydrogen-rich Wolf-Rayet stars
Lirias (KU Leuven)·2025· 1 citedOpen Access
The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
Astronomy and Astrophysics·2025· 2 citedOpen Access
The black hole–pair instability boundary for high stellar rotation
Monthly Notices of the Royal Astronomical Society·2025· 2 citedOpen Access
The black hole - pair instability boundary for high stellar rotation
arXiv (Cornell University)·2025Open Access
The wind properties of O-type stars at sub-SMC metallicity
Astronomy and Astrophysics·2025· 2 citedOpen Access
Binarity at LOw Metallicity (BLOeM)
Astronomy and Astrophysics·2025· 10 citedOpen Access
Binarity at LOw Metallicity (BLOeM)
Astronomy and Astrophysics·2025· 2 citedOpen Access
page 1 of 27Next →

Frequent Co-authors

A. de Koter(28), N. Langer(24), C. J. Evans(18), A. Herrero(16), D. J. Lennon(16), H. Sana(15), P. A. Crowther(15), G. Gräfener(15), J. Maíz Apellániz(14), W. D. Taylor(13), S. E. de Mink(12), J. Puls(12), F. Najarro(11), S. Simón‐Díaz(9), J. M. Bestenlehner(9), V. Hénault-Brunet(8), N. R. Walborn(8), I. Brott(7), O. H. Ramírez-Agudelo(7), J. E. Drew(7)