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W. Hamann

59 papers hereh-index 303.5k citations219 works total

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

author position
  • first author4
  • middle author24
  • last author24

Across the 52 of 59 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR40
  • astro-ph15
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • W. Hamann — 36 papers, h 10
  • W. Hamann — 30 papers, h 17
  • W. Hamann — 1 paper, h 1

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
20012022
most citedThe Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation

328 citations · 3.2k across the 59 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.SR2014★ 35 cited

A new type of X-ray pulsar

Lidia M. Oskinova, Yael Naze, Helge Todt +4

X-ray emission from stars much more massive than the Sun was discovered only 35 years ago. Such stars drive fast stellar winds where shocks can develop, and it is commonly assumed…

astro-ph.SR2014★ 30 cited

The Wolf-Rayet stars in M31: I. Analysis of the late-type WN stars

Andreas Sander, Helge Todt, Rainer Hainich +1

Context: Comprehensive studies of Wolf-Rayet stars were performed in the past for the Galactic and the LMC population. The results revealed significant differences, but also unexpe…

astro-ph.SR2014★ 49 cited

The impact of rotation on the line profiles of Wolf-Rayet stars

Tomer Shenar, Wolf-Rainer Hamann, Helge Todt

Massive Wolf-Rayet stars are recognized today to be in a very common, but short, evolutionary phase of massive stars. While our understanding of Wolf-Rayet stars has increased dram…

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