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C. Aerts

18 papers hereh-index 7333 citations23 works total

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

author position
  • middle author5
  • last author8

Across the 13 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR17
  • astro-ph.IM1
same name
  • C. Aerts — 165 papers, h 67
  • C. Aerts — 74 papers, h 32
  • C. Aerts — 70 papers, h 30
  • C. Aerts — 20 papers, h 6
  • C. Aerts — 9 papers
  • C. Aerts — 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

activity
20172026
most citedForward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection

101 citations · 552 across the 18 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.SR2018★ 95 cited

On the photometric detection of Internal Gravity Waves in upper main-sequence stars I. Methodology and application to CoRoT targets

D. M. Bowman, C. Aerts, C. Johnston +8

Context. Main sequence stars with a convective core are predicted to stochastically excite Internal Gravity Waves (IGWs), which effectively transport angular momentum throughout th…

astro-ph.SR2018★ 101 cited

Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection

C. Aerts, G. Molenberghs, M. Michielsen +13

We propose a methodological framework to perform forward asteroseismic modeling of stars with a convective core, based on gravity-mode oscillations. These probe the near-core regio…

astro-ph.SR2018★ 90 cited

Forward seismic modelling of the pulsating magnetic B-type star HD 43317

B. Buysschaert, C. Aerts, D. M. Bowman +5

The large-scale magnetic fields detected at the surface of about 10% of hot stars extend into the stellar interior, where they may alter the structure. Deep inner regions of stars…

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