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researcher

R. Lefever

30 papers hereh-index 565 citations33 works total

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

author position
  • first author4
  • middle author25

Across the 29 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR24
  • astro-ph.GA3
  • physics.ed-ph1
  • physics.gen-ph1
  • physics.pop-ph1
same name
  • R. Lefever — 2 papers, h 33

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
20222026
most citedX-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

61 citations · 297 across the 29 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2025★ 1 cited

Can Wolf-Rayet stars be the missing ingredient to explain high-z He II ionizing radiation?

G. González-Torà, A. A. C. Sander, E. Egorova +7

Classical Wolf-Rayet (WR) stars are hot, massive stars with depleted hydrogen. At low metallicities (Z), WN3-type WR stars have relatively thin winds and are major sources of ioniz…

astro-ph.GA2025★ 3 cited

Mass loading of outflows from evolving Young Massive Clusters

C. J. K. Larkin, C. Hawcroft, J. Mackey +3

Feedback from Young Massive Clusters (YMCs) is an important driver of galaxy evolution. In the first few Myr, mechanical feedback is dominated by collective effects of the massive…

astro-ph.GA2025★ 4 cited

Extremely iron-poor O-type stars in the Magellanic Bridge

E. C. Schösser, V. Ramachandran, A. A. C. Sander +7

To study stars analogous to those in the early Universe with redshift z > 3, we need to probe environments with low metallicities. Until recently, massive O-type stars with metalli…

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