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D. J. Hillier

3 papers hereh-index 6277 citations25 works total

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
same name
  • D. J. Hillier — 15 papers
  • D. J. Hillier — 2 papers, h 9
  • D. J. Hillier — 2 papers, h 3
  • D. J. Hillier — 1 paper, h 0

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

most citedNo breakdown of the radiatively-driven wind theory in low-metallicity environments

57 citations · 74 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024★ 17 cited

X-Shooting ULLYSES: Massive stars at low metallicity. IV. Spectral analysis methods and exemplary results for O stars

A. A. C. Sander, J. -C. Bouret, M. Bernini-Peron +26

CONTEXT: The spectral analysis of hot, massive stars is a fundamental astrophysical method to obtain their intrinsic properties and their feedback. Quantitative spectroscopy for ho…

astro-ph.SR2024

X-Shooting ULLYSES: Massive stars at low metallicity -- V. Effect of metallicity on surface abundances of O stars

F. Martins, J. -C. Bouret, D. J. Hillier +10

Massive stars rotate faster, on average, than lower mass stars. Stellar rotation triggers hydrodynamical instabilities which transport angular momentum and chemical species from th…

astro-ph.SR2015★ 57 cited

No breakdown of the radiatively-driven wind theory in low-metallicity environments

J. -C. Bouret, T. Lanz, D. J. Hillier +3

We present a spectroscopic analysis of HST/COS observations of three massive stars in the low metallicity dwarf galaxies IC 1613 and WLM. These stars, were previously observed with…

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