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K. Pouilly

3 papers here

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

author position
  • first author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3

identity via Semantic Scholar / OpenAlex

most citedAccretion process, magnetic fields, and apsidal motion in the pre-main sequence binary DQ Tau

1 citations · 1 across the 1 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2022★ 1 cited

Accretion process, magnetic fields, and apsidal motion in the pre-main sequence binary DQ Tau

Kim Pouilly, Oleg Kochukhov, Ágnes Kóspál +3

Classical T Tauri stars (CTTSs) are young stellar objects that accrete materials from their accretion disc influenced by their strong magnetic field. The magnetic pressure truncate…

astro-ph.SR2020

Investigating the magnetospheric accretion process in the young pre-transitional disk system DoAr 44 (V2062~Oph). A multiwavelength interferometric, spectropolarimetric, and photometric observing campaign

J. Bouvier, E. Alecian, S. H. P. Alencar +13

Young stars interact with their accretion disk through their strong magnetosphere. We investigate the magnetospheric accretion process in the young stellar system DoAr 44. We monit…

astro-ph.SR2020

Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tau

K. Pouilly, J. Bouvier, E. Alecian +7

Context. Classical T Tauri stars (cTTs) are pre-main sequence stars surrounded by an accretion disk. They host a strong magnetic field, and both magnetospheric accretion and ejecti…

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