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researcher

G. Gräfener

37 papers hereh-index 333.8k citations105 works total

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

author position
  • sole author1
  • first author5
  • middle author24
  • last author1

Across the 31 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR32
  • astro-ph2
  • astro-ph.GA2
  • astro-ph.HE1
same name
  • G. Gräfener — 14 papers, h 0
  • 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
20062021
most citedThe Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation

328 citations · 3.4k across the 37 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.SR2011★ 183 cited

Stellar envelope inflation near the Eddington limit. Implications for the radii of Wolf-Rayet stars and luminous blue variables

G. Gräfener, S. P. Owocki, J. S. Vink

(shortened) It has been proposed that the envelopes of luminous stars may be subject to substantial radius inflation. The inflation effect has been discussed in relation to the rad…

astro-ph.SR2011★ 24 cited

In pursuit of gamma-ray burst progenitors: the identification of a sub-population of rotating Wolf-Rayet stars

Jorick S. Vink, G. Graefener, T. J. Harries

Long gamma-ray bursts involve the most powerful cosmic explosions since the Big Bang. Whilst it has been established that GRBs are related to the death throes of massive stars, the…

astro-ph.SR2011★ 61 cited

The spectral variability and magnetic field characteristics of the Of?p star HD 148937

G. A. Wade, J. Grunhut, G. Graefener +11

We report magnetic and spectroscopic observations and modeling of the Of?p star HD 148937 within the context of the MiMeS LP at the CFHT. Thirty-two high signal-to-noise ratio circ…

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