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researcher

H. Méheut

4 papers here

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

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

activity
20122024
most citedRossby Wave Instability in three dimensional discs

69 citations · 125 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2024★ 2 cited

Reduction of dust radial drift by turbulence in protoplanetary disks

Fabiola Antonietta Gerosa, Jérémie Bec, Héloïse Méheut +1

Dust particles in protoplanetary disks, lacking support from pressure, rotate at velocities exceeding those of the surrounding gas. Consequently, they experience a head-wind from t…

astro-ph.EP2014★ 18 cited

Planet-vortex interaction:How a vortex can shepherd a planetary embryo

S. Ataiee, C. P. Dullemond, W. Kley +2

Context: Anticyclonic vortices are considered as a favourable places for trapping dust and forming planetary embryos. On the other hand, they are massive blobs that can interact gr…

astro-ph.SR2013★ 36 cited

How strong are the Rossby vortices?

H. Meheut, R. V. E. Lovelace, D. Lai

The Rossby wave instability, associated with density bumps in differentially rotating discs, may arise in several different astrophysical contexts, such as galactic or protoplaneta…

astro-ph.EP2012★ 69 cited

Rossby Wave Instability in three dimensional discs

H. Meheut, C. Yu, D. Lai

The Rossby wave instability (RWI) is a promising mechanism for producing large-scale vortices in protoplanetary discs. The instability operates around a density bump in the disc, a…

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