Christopher H. Evans

Astronomy and Astrophysics · 2002–2012

A researcher in the Science corpus: 11 papers; trusts 14 researchers and is trusted by 32 researchers here, as inferred from the citation graph.

Subfields

• Astronomy and Astrophysics — 141 citations into it; #1,828 of 10,964 by trust here, #1,980 by citations
• Instrumentation — 62 citations into it; #1,388 of 3,502 by trust here, #1,362 by citations
• Atomic and Molecular Physics, and Optics — 8 citations into it

Whom Christopher H. Evans trusts overall

Their strongest outbound trust, strongest first, inferred from their citations.

1. P. Crowther
2. D. John Hillier
3. R. Kudritzki
4. J. Bouret
5. Tim Harries
6. T. Lanz
7. J. Puls
8. Andre Maeder
9. D. Lennon
10. A. Pauldrach

Who trusts Christopher H. Evans overall

1. N. Smith
2. J. Puls
3. I. Hunter
4. Selma de Mink
5. N. Giacobbo
6. N. Langer
7. S. Smartt
8. Fabrice Martins
9. Michela Mapelli
10. P. Dufton

Papers from Christopher H. Evans's perspective

Ordered by how strongly the researchers Christopher H. Evans trusts endorse each paper. Same corpus, a different order for every researcher.

1. WINDS FROM HOT STARS
2. Stellar evolution with rotation. VII. - Low metallicity models and the blue to red supergiant ratio in the SMC
3. A New Spectral Classification System for the Earliest O Stars: Definition of Type O2
4. A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69
5. Radiation-driven winds of hot luminous stars - XIII. A description of NLTE line blocking and blanketing towards realistic models for expanding atmospheres
6. A new calibration of stellar parameters of Galactic O stars
7. Revised Stellar Temperatures for Magellanic Cloud O Supergiants from Far Ultraviolet Spectroscopic Explorer and Very Large Telescope UV-Visual Echelle Spectrograph Spectroscopy
8. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
9. Line-driven Winds, Ionizing Fluxes, and Ultraviolet Spectra of Hot Stars at Extremely Low Metallicity. I. Very Massive O Stars
10. Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties

Their papers

• Binary Interaction Dominates the Evolution of Massive Stars (2012) — 1,465 citations
• The VLT-FLAMES Tarantula survey (2009) — 457 citations
• The VLT-FLAMES survey of massive stars: constraints on stellar evolution from the chemical compositions of rapidly rotating Galactic and Magellanic Cloud B-type stars (2009) — 160 citations
• The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds , (2007) — 148 citations
• The VLT FLAMES Survey of Massive Stars: Rotation and Nitrogen Enrichment as the Key to Understanding Massive Star Evolution (2007) — 141 citations
• The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars (2007) — 246 citations
• The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region (2006) — 157 citations
• The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611 ⋆ (2005) — 140 citations
• Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346 (2003) — 209 citations
• A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69 (2003) — 151 citations
• Revised Stellar Temperatures for Magellanic Cloud O Supergiants from Far Ultraviolet Spectroscopic Explorer and Very Large Telescope UV-Visual Echelle Spectrograph Spectroscopy (2002) — 144 citations