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D. J. Hillier

4 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
  • last author1

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

fields
  • astro-ph.SR4
same name
  • D. J. Hillier — 2 papers, h 9

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
20242026
collaborators

4 papers

astro-ph.SR2026

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI

Calum Hawcroft, David R. Law, Linda J. Smith +8

We investigate the presence of high ionization fine-structure emission lines across a range of 22 OB-type stars observed with JWST-MIRI as part of calibration programmes and the WI…

astro-ph.SR2025

Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Br-alpha Spectroscopy

Miriam Garcia, Alexander W. Fullerton, Francisco Najarro +12

Mass loss is a key physical process in the evolution of massive stars, the impact of which propagates into galactic evolution, population synthesis models, the interpretation of hi…

astro-ph.SR2025

X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud

Sarah A. Brands, Frank Backs, Alex de Koter +23

Mass loss governs the evolution of massive stars and shapes the stellar surroundings. To quantify the impact of the stellar winds we need to know the exact mass-loss rates; however…

astro-ph.SR2024

The Nature of a Recently Discovered Wolf-Rayet Binary: Archetype of Stripping?

Philip Massey, Kathryn F. Neugent, Nidia I. Morrell +2

LMCe055-1 was recently discovered in a survey for WRs in the Large Magellanic Cloud, and classified as a WN4/O4, a lower excitation version of the WN3/O3 class discovered as part o…

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