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A. de Koter

151 papers hereh-index 12941 citations36 works total

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

author position
  • middle author121
  • last author14

Across the 135 of 151 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR119
  • astro-ph12
  • astro-ph.GA12
  • astro-ph.HE4
  • astro-ph.IM2
  • astro-ph.EP1
same name
  • A. de Koter — 32 papers
  • A. de Koter — 5 papers
  • A. de Koter — 2 papers
  • A. de Koter — 2 papers
  • A. de Koter — 2 papers, h 11
  • A. de Koter — 1 paper

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
19962026
most citedMass-loss predictions for O and B stars as a function of metallicity

1.7k citations · 12.2k across the 150 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.SR2020★ 31 cited

Atomium: A high-resolution view on the highly asymmetric wind of the AGB star Pi1 Gruis. I. First detection of a new companion and its effect on the inner wind

Ward Homan, Miguel Montarges, Bannawit Pimpanuwat +35

The nebular circumstellar environments of cool evolved stars are known to harbour a rich morphological complexity of gaseous structures on different length scales. A large part of…

astro-ph.SR2020★ 132 cited

(Sub)stellar companions shape the winds of evolved stars

L. Decin, M. Montargès, A. M. S. Richards +32

Binary interactions dominate the evolution of massive stars, but their role is less clear for low- and intermediate-mass stars. The evolution of a spherical wind from an asymptotic…

astro-ph.SR2020★ 112 cited

The R136 star cluster dissected with Hubble Space Telescope/STIS. II. Physical properties of the most massive stars in R136

Joachim M. Bestenlehner, Paul A. Crowther, Saida M. Caballero-Nieves +11

We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of the Large Magellanic Cloud. Our sample was observed with STIS aboard the Hubble…

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