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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 — 37 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 2013Show all

1 paper · 1 filter

astro-ph.SR2013★ 34 cited

One of the most massive stars in the Galaxy may have formed in isolation

L. M. Oskinova, M. Steinke, W. -R. Hamann +3

Very massive stars, 100 times heavier than the sun, are rare. It is not yet known whether such stars can form in isolation or only in star clusters. The answer to this question is…

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