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W. Hamann

4 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 author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.SR1
same name
  • W. Hamann — 14 papers, h 30
  • W. Hamann — 1 paper, h 10

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
20042009
most citedThe Quintuplet Cluster I. A K-band spectral catalog of stellar sources

63 citations · 102 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2009★ 34 cited

Discovery of X-ray Emission from the Wolf-Rayet star WR142 of oxygen subtype

L. M. Oskinova, W. -R. Hamann, A. Feldmeier +2

We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR142 with the XMM-Newton X-ray telescope. Being of spectral subtype WO2, WR142 is a massive s…

astro-ph2008★ 63 cited

The Quintuplet Cluster I. A K-band spectral catalog of stellar sources

A. Liermann, W. -R. Hamann, L. M. Oskinova

Three very massive clusters are known to reside in the Galactic Center region, the Arches cluster, the Quintuplet cluster and the Central parsec cluster. We obtained spectroscopic…

astro-ph2007★ 5 cited

Revised element abundances for WC-type central stars

H. Todt, G. Gräfener, W. -R. Hamann

According to previous spectral analyses of Wolf-Rayet type central stars, late [WC] subtypes show systematically higher carbon-to-helium abundance ratios than early [WC] subtypes.…

astro-ph2004

X-ray emission lines from inhomogeneous stellar winds

L. M. Oskinova, A. Feldmeier, W. -R. Hamann

It is commonly adopted that X-rays from O stars are produced deep inside the stellar wind, and transported outwards through the bulk of the expanding matter which attenuates the ra…

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