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W. Hamann

30 papers hereh-index 17801 citations41 works total

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

author position
  • middle author21
  • last author5

Across the 26 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR19
  • astro-ph6
  • astro-ph.GA3
  • astro-ph.HE2
same name
  • W. Hamann — 59 papers, h 30
  • W. Hamann — 37 papers, h 10
  • 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
20032026
most citedEarly magnetic B-type stars: X-ray emission and wind properties

118 citations · 1k across the 30 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

3 papers · 2 filters

astro-ph2003★ 17 cited

Comprehensive modelling of the planetary nebula LMC-SMP 61 and its [WC]-type central star

G. Stasińska, G. Gräfener, M. Peña +3

We present a comprehensive study of the Magellanic Cloud planetary nebula SMP 61 and of its nucleus, a Wolf-Rayet type star classified [WC 5-6]. We have performed a detailed spectr…

astro-ph2003★ 75 cited

The Conspicuous Absence of X-ray Emission from Carbon-Enriched Wolf-Rayet Stars

L. M. Oskinova, R. Ignace, W. -R. Hamann +2

The carbon-rich WC5 star WR 114 was not detected during a 15.9 ksec XMM-Newton observation, implying an upper limit to the X-ray luminosity of Lx < 2.5*10^{30} erg/s and to the X-r…

astro-ph2003★ 112 cited

X-ray line emission from a fragmented stellar wind

Achim Feldmeier, Lida Oskinova, Wolf-Rainer Hamann

We discuss X-ray line formation in dense O star winds. A random distribution of wind shocks is assumed to emit X-rays that are partially absorbed by cooler wind gas. The cool gas r…

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