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researcher

J. Vink

202 papers hereh-index 487.8k citations284 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author27
  • first author31
  • middle author74
  • last author45

Across the 177 of 202 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR123
  • astro-ph50
  • astro-ph.GA13
  • astro-ph.IM8
  • astro-ph.HE7
  • astro-ph.CO1
same name
  • J. Vink — 318 papers, h 58
  • J. Vink — 73 papers, h 20
  • J. Vink — 54 papers, h 20
  • J. Vink — 24 papers, h 10
  • J. Vink — 23 papers, h 7
  • J. Vink — 23 papers, h 6

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19992026
most citedMass-loss predictions for O and B stars as a function of metallicity

1.7k citations · 12.3k across the 196 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.SR2026

The physical origin of the maximum stellar size

Gautham N. Sabhahit, Jorick S. Vink

One might expect the most massive stars to also be the largest by size, yet they are not, and this has puzzled astronomers for decades. The Eddington limit sets an upper bound to s…

astro-ph.SR2026

Hydrodynamical mass-loss rates for Very Massive Stars II. New theoretical mass-loss predictions at solar metallicity (Z = 0.02)

Gautham N. Sabhahit, Jorick S. Vink, Andreas A. C. Sander

The evolutionary pathways and ultimate fates of very massive stars are governed primarily by mass loss through radiatively driven winds. We present a new theoretical mass-loss pres…

astro-ph.SR2026

The winds of OBA hypergiants and luminous blue variables: Dynamically-consistent atmosphere models reveal multiple wind regimes

Matheus Bernini-Peron, Andreas A. C. Sander, Gautham N. Sabhahit +3

OBA hypergiants (OBAHGs) are evolved massive stars with notable wind features in their optical spectrum. Located at the cool edge of the line-driven wind regime, many are candidate…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.