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T. Ceulemans

2 papers here

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

author position
  • middle author1
  • last author1

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
same name
  • T. Ceulemans — 1 paper, h 2

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 cited3D simulations of AGB stellar winds -- II. Ray-tracer implementation and impact of radiation on the outflow morphology

14 citations · 14 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2024

Modelling predicts a molecule-rich disk around the AGB star L2 Puppis

M. Van de Sande, C. Walsh, T. Danilovich +2

The nearby oxygen-rich AGB star L2 Pup hosts a well-studied nearly edge-on disk. To date, disks around AGB stars have not been chemically studied in detail. By combining a paramete…

astro-ph.SR2023★ 14 cited

3D simulations of AGB stellar winds -- II. Ray-tracer implementation and impact of radiation on the outflow morphology

Mats Esseldeurs, Lionel Siess, Frederik De Ceuster +6

Stars with an initial mass below ~ 8 Msun evolve through the asymptotic giant branch (AGB) phase, during which they develop strong stellar winds. Recent observations have revealed…

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