W. Hamann
Astronomy and Astrophysics · 2002–2014
A researcher in the Science corpus: 8 papers; trusts 31 researchers and is trusted by 51 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 89 citations into it; #931 of 10,964 by trust here, #4,064 by citations
- Instrumentation — 39 citations into it; #690 of 3,502 by trust here, #2,190 by citations
Whom W. Hamann trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- G. Gräfener
- E. Fitzpatrick
- P. Crowther
- L. Koesterke
- D. Figer
- Philip Massey
- D. John Hillier
- Andre Maeder
- S. Owocki
- J. Puls
Who trusts W. Hamann overall
- G. Graefener
- A. Sander
- R. Hainich
- G. Meynet
- S. Ekström
- C. Georgy
- J. Groh
- C. Leitherer
- S. Smartt
- H. Todt
Papers from W. Hamann's perspective
Ordered by how strongly the researchers W. Hamann trusts endorse each paper. Same corpus, a different order for every researcher.
- A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69
- WINDS FROM HOT STARS
- The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
- Stellar evolution with rotation. VII. - Low metallicity models and the blue to red supergiant ratio in the SMC
- Stellar and wind properties of LMC WC4 stars A metallicity dependence for Wolf-Rayet mass-loss rates ?
- Massive Stars in the Local Group: Implications for Stellar Evolution and Star Formation
- Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346
- Stellar evolution with rotation XI. Wolf-Rayet star populations at different metallicities
- Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties
- Line-driven Winds, Ionizing Fluxes, and Ultraviolet Spectra of Hot Stars at Extremely Low Metallicity. I. Very Massive O Stars
Their papers
- The Wolf-Rayet stars in the Large Magellanic Cloud - A comprehensive analysis of the WN class (2014) — 135 citations
- The Galactic WC stars Stellar parameters from spectral analyses indicate a new evolutionary sequence (2012) — 170 citations
- Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit (2008) — 155 citations
- Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates (2007) — 170 citations
- The Galactic WN stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolut (2006) — 257 citations
- The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611 ⋆ (2005) — 140 citations
- Grids of model spectra for WN stars, ready for use (2004) — 155 citations
- Line-blanketed model atmospheres for WR stars (2002) — 219 citations