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researcher

G. Gräfener

14 papers hereh-index 00 citations0 works total

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

author position
  • first author1
  • middle author10
  • last author1

Across the 12 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR11
  • astro-ph1
  • astro-ph.HE1
  • physics.gen-ph1
same name
  • G. Gräfener — 37 papers, h 33
  • G. Gräfener — 11 papers
  • G. Gräfener — 1 paper, 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
20032026
most citedWind modelling of very massive stars up to 300 solar masses

191 citations · 731 across the 14 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.SR2011

Wind Models for Very Massive Stars in the Local Universe

Jorick S. Vink, J. M. Bestenlehner, G. Graefener +2

Some studies have claimed the existence of a stellar upper-mass limit of 150 Msun. A factor that is often overlooked concerns the issue that there might be a significant difference…

astro-ph.SR2011★ 175 cited

The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Gamma-dependence of Wolf-Rayet type mass loss

G. Gräfener, J. S. Vink, A. de Koter +1

The most massive stars are thought to be hydrogen-rich Wolf-Rayet stars of late spectral subtype (WNh stars). In previous theoretical studies the enhanced mass loss of these stars…

astro-ph.SR2011★ 191 cited

Wind modelling of very massive stars up to 300 solar masses

Jorick S. Vink, L. E. Muijres, B. Anthonisse +3

Some studies have claimed a universal stellar upper-mass limit of 150 Msun. A factor that is often overlooked is that there might be a difference between the current and initial ma…

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