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W. Homan

35 papers hereh-index 16748 citations62 works total

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

author position
  • first author7
  • middle author23
  • last author1

Across the 31 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR33
  • astro-ph.IM2

identity via Semantic Scholar / OpenAlex

activity
20152023
most cited(Sub)stellar companions shape the winds of evolved stars

132 citations · 1.2k across the 35 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.IM2019★ 29 cited

Magritte, a modern software library for 3D radiative transfer: I. Non-LTE atomic and molecular line modelling

Frederik De Ceuster, Ward Homan, Jeremy Yates +3

Radiative transfer is a key component in almost all astrophysical and cosmological simulations. We present Magritte: a modern open-source software library for 3D radiative transfer…

astro-ph.SR2019★ 28 cited

NOEMA maps the CO J=2−1 environment of the red supergiant μ Cep

M. Montargès, W. Homan, D. Keller +8

Red supergiant stars are surrounded by a gaseous and dusty circumstellar environment created by their mass loss which spreads heavy elements into the interstellar medium. The struc…

astro-ph.SR2019★ 42 cited

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

L. Decin, W. Homan, T. Danilovich +12

In 1981, the idea of a superwind that ends the life of cool giant stars was proposed. Extreme OH/IR-stars develop superwinds with the highest mass-loss rates known so far, up to a…

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