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M. Rieutord

67 papers hereh-index 374.1k citations188 works total

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

author position
  • sole author8
  • first author11
  • middle author18
  • last author25

Across the 62 of 67 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR38
  • astro-ph20
  • physics.flu-dyn7
  • gr-qc1
  • physics.comp-ph1
same name
  • M. Rieutord — 16 papers
  • M. Rieutord — 9 papers, h 7
  • M. Rieutord — 9 papers, h 1
  • M. Rieutord — 5 papers, h 4
  • M. Rieutord — 2 papers, h 4

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
20002023
most citedGravity darkening in rotating stars

267 citations · 2.4k across the 65 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

astro-ph.SR2012★ 115 cited

Self-consistent 2D models of fast rotating early-type star

F. Espinosa Lara, M. Rieutord

This work aims at presenting the first two-dimensional models of an isolated rapidly rotating star that include the derivation of the differential rotation and meridional circulati…

astro-ph.SR2012★ 35 cited

Gravity Darkening in Binary Stars

Francisco Espinosa Lara, Michel Rieutord

Context.Interpretation of light curves of many types of binary stars requires the inclusion of the (cor)relation between surface brightness and local effective gravity. Until recen…

physics.flu-dyn2012★ 39 cited

On the excitation of inertial modes in an experimental spherical Couette flow

Michel Rieutord, Santiago Andres Triana, Daniel S. Zimmerman +1

Spherical Couette flow (flow between concentric rotating spheres) is one of flows under consideration for the laboratory magnetic dynamos. Recent experiments have shown that such f…

astro-ph.SR2012★ 18 cited

Ab initio modelling of steady rotating stars

Michel Rieutord, Francisco Espinosa Lara

Modelling isolated rotating stars at any rotation rate is a challenge for the next generation of stellar models. These models will couple dynamical aspects of rotating stars, like…

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